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|
| 1 |
+
arXiv:2301.13239v1 [math.QA] 30 Jan 2023
|
| 2 |
+
Periodic Y-systems and Nahm sums: the rank 2 case
|
| 3 |
+
Yuma Mizuno
|
| 4 |
+
Abstract
|
| 5 |
+
We classify periodic Y-systems of rank 2 satisfying the symplectic property. We find
|
| 6 |
+
that there are six such Y-systems. In all cases, the periodicity follows from the existence
|
| 7 |
+
of two reddening sequences associated with the time evolution of the Y-systems in positive
|
| 8 |
+
and negative directions, which gives rise to quantum dilogarithm identities associated with
|
| 9 |
+
Donaldson-Thomas invariants. We also consider q-series called the Nahm sums associated
|
| 10 |
+
with these Y-systems. We see that they are included in Zagier’s list of rank 2 Nahm sums
|
| 11 |
+
that are likely to be modular functions. It was recently shown by Wang that they are indeed
|
| 12 |
+
modular functions.
|
| 13 |
+
1
|
| 14 |
+
Introduction
|
| 15 |
+
1.1
|
| 16 |
+
Background
|
| 17 |
+
The Y-system is a system of algebraic relations satisfied by coefficients of a cluster algebra,
|
| 18 |
+
which has the following form:
|
| 19 |
+
Yi(u)Yi(u − ri) =
|
| 20 |
+
�
|
| 21 |
+
j∈I
|
| 22 |
+
ri−1
|
| 23 |
+
�
|
| 24 |
+
p=1
|
| 25 |
+
Yj(u − p)[nij;p]+�
|
| 26 |
+
1 + Yj(u − p)
|
| 27 |
+
�−nij;p
|
| 28 |
+
(1.1)
|
| 29 |
+
where I is a finite index set, Yi(u) for i ∈ I, u ∈ Z are commuting variables, ri ∈ Z≥1, and
|
| 30 |
+
nij;p ∈ Z. We also use the notation [n]+ := max(0, n).
|
| 31 |
+
Such equations are first discovered
|
| 32 |
+
by Zamolodchikov in the study of thermodynamic Bethe ansats [36], prior to the discovery of
|
| 33 |
+
cluster algebras by Fomin and Zelevinsky [7]. The most striking feature of Zamolodchikov’s Y-
|
| 34 |
+
systems, as well as their generalizations [22, 30] defined shortly after the Zamolodchikov’s work,
|
| 35 |
+
is that they are periodic, which was fully proved by applying the theory of cluster algebras
|
| 36 |
+
[9, 10, 15, 16, 21].
|
| 37 |
+
A systematic treatment of the Y-systems in the general setting of cluster algebras, including
|
| 38 |
+
the Y-systems arising from the thermodynamic Bethe ansatz as spacial cases, was given by
|
| 39 |
+
Nakanishi [27]. This approach was further developed in [24], and it was shown that the algebraic
|
| 40 |
+
relation (1.1) arises from a cluster algebra if and only if the data ri, nij;p have a certain symplectic
|
| 41 |
+
property. This allows the “axiomatic” study of Y-systems without explicitly referring to cluster
|
| 42 |
+
algebras. In this general setting, however, the Y-system is typically not periodic, and so the
|
| 43 |
+
study of periodic Y-systems as a generalization of Zamolodchikov’s Y-systems would be further
|
| 44 |
+
developed. In particular, the classification problem for periodic Y-systems is a challenging open
|
| 45 |
+
problem (see the last comments in [27, Section 3]).
|
| 46 |
+
There are several classification results in the literature. Fomin and Zelevinsky [10] showed
|
| 47 |
+
that the classification when ri = 2, nij;p ≤ 0, and nii;p = 0 for any i, j, p coincides with the
|
| 48 |
+
Cartan-Killing classification. Galashin and Pylyavskyy [12] generalized this result to show that
|
| 49 |
+
the classification when ri = 2 and nii;p = 0 for any i, p coincides with the classification of ADE
|
| 50 |
+
bigraphs of Stembridge [31]. On the other hand, the situation is more complicated when ri > 2
|
| 51 |
+
for some i, and so far there has been no comprehensive classification results except when |I| = 1
|
| 52 |
+
1
|
| 53 |
+
|
| 54 |
+
where it is not difficult to give a complete classification thanks to the work by Fordy and Marsh
|
| 55 |
+
[11] (e.g. see [24, Example 5.6]).
|
| 56 |
+
In this paper, we make a first attempt to give a classification result involving the case ri > 2
|
| 57 |
+
for some i. Precisely, we classify the periodic Y-systems of the form (1.1) with |I| = 2 satisfying
|
| 58 |
+
the symplectic property. We would like to emphasize that we consider general ri, nij;p in the
|
| 59 |
+
classification. The result is given in the next section.
|
| 60 |
+
We also discuss the relation to Nahm’s conjecture on q-series [26, 35] in Section 1.3.
|
| 61 |
+
1.2
|
| 62 |
+
Main result
|
| 63 |
+
Let I be a finite set.
|
| 64 |
+
We denote by Y0 the set of pairs (r, n) where r = (ri)i∈I and n =
|
| 65 |
+
(nij;p)i,j∈I,p∈N are families of integers satisfying ri ≥ 1 for any i and
|
| 66 |
+
n±
|
| 67 |
+
ij;p = 0 unless 0 < p < ri
|
| 68 |
+
(1.2)
|
| 69 |
+
for any i, j, p.
|
| 70 |
+
Definition 1.1. Let (r, n) ∈ Y0. Let P be a semifield, and (Yi(u))i∈I,u∈Z be a family of elements
|
| 71 |
+
in P. We say that (Yi(u)) satisfies the Y-system associated with the pair (r, n) if the relation
|
| 72 |
+
(1.1) holds for any i, u. The equation (1.1) itself is called the Y-system associated with (r, n).
|
| 73 |
+
We also say that (Yi(u)) is a solution of the Y-system if it satisfies the Y-system.
|
| 74 |
+
It is useful to think a pair (r, n) ∈ Y0 as a triple of matrices with polynomial entries by the
|
| 75 |
+
map (r, n) �→ (N0(z), N+(z), N−(z)) : Y0 → (MatI×I N[z])3 defined by
|
| 76 |
+
N0(z) := diag(1 + zri)i∈I,
|
| 77 |
+
N±(z) :=
|
| 78 |
+
� �
|
| 79 |
+
p∈N
|
| 80 |
+
n±
|
| 81 |
+
ij;pzp
|
| 82 |
+
�
|
| 83 |
+
i,j∈I
|
| 84 |
+
(1.3)
|
| 85 |
+
where we set n±
|
| 86 |
+
ij;p := [±nij;p]+. We also define the map (r, n) �→ A±(z) : Y0 → (MatI×I Z[z])2
|
| 87 |
+
by A±(z) := N0(z) − N±(z). Since this map is injective by the condition (1.2), we will identify
|
| 88 |
+
Y0 with the image of this map. For example, we will use the term “the Y-system associated
|
| 89 |
+
with A±(z) ∈ Y0”.
|
| 90 |
+
Definition 1.2. We say that A±(z) ∈ Y0 satisfies the symplectic property if
|
| 91 |
+
A+(z)A−(z−1)T = A−(z)A+(z−1)T,
|
| 92 |
+
(1.4)
|
| 93 |
+
where T is the transpose of a matrix. We denote by Y the subset of Y0 consisting of pairs
|
| 94 |
+
satisfying the symplectic property.
|
| 95 |
+
The pair A±(z) ∈ Y0 satisfies the simplectic property if and only if the Y-system associated
|
| 96 |
+
with A±(z) ∈ Y0 is realized as the exchange relations of coefficients in a cluster algebra [24].
|
| 97 |
+
We review this fact in Section 2.1.
|
| 98 |
+
Definition 1.3. We say that a solution of a Y-system is periodic if there is a positive integer
|
| 99 |
+
Ω > 0 such that Yi(u + Ω) = Yi(u) for any i, u.
|
| 100 |
+
Definition 1.4. We say that a pair A±(z) ∈ Y is of finite type if any solution (in any semifield)
|
| 101 |
+
of the Y-system associated with this pair is periodic. In this case, we also say that Y-system
|
| 102 |
+
itself is periodic.
|
| 103 |
+
The purpose of this paper is to classify periodic Y-systems of rank 2. Before stating the
|
| 104 |
+
result, we give a few remarks. We say that A±(z) ∈ YI is decomposable if it is a direct sum
|
| 105 |
+
of some A′
|
| 106 |
+
±(z) ∈ YI′ and A′′
|
| 107 |
+
±(z) ∈ YI′′ with nonempty I′ and I′′. We say that A±(z) ∈ YI
|
| 108 |
+
is indecomposable if it is not decomposable. It is enough to consider indecomposable pairs in
|
| 109 |
+
the classification. We also note that A±(z) is of finite type if and only if A±(z)op := A∓(z) is
|
| 110 |
+
of finite type by the correspondence between solutions Yi(u) �→ Yi(u)−1. The main results are
|
| 111 |
+
summarized as follows:
|
| 112 |
+
2
|
| 113 |
+
|
| 114 |
+
A+(z)
|
| 115 |
+
A−(z)
|
| 116 |
+
h+
|
| 117 |
+
h−
|
| 118 |
+
�
|
| 119 |
+
1 + z2
|
| 120 |
+
−z
|
| 121 |
+
−z
|
| 122 |
+
1 + z2
|
| 123 |
+
�
|
| 124 |
+
�
|
| 125 |
+
1 + z2
|
| 126 |
+
0
|
| 127 |
+
0
|
| 128 |
+
1 + z2
|
| 129 |
+
�
|
| 130 |
+
3
|
| 131 |
+
2
|
| 132 |
+
(1)
|
| 133 |
+
�
|
| 134 |
+
1 + z2
|
| 135 |
+
−z
|
| 136 |
+
−z − z5
|
| 137 |
+
1 + z6
|
| 138 |
+
�
|
| 139 |
+
�
|
| 140 |
+
1 + z2
|
| 141 |
+
0
|
| 142 |
+
−z3
|
| 143 |
+
1 + z6
|
| 144 |
+
�
|
| 145 |
+
8
|
| 146 |
+
6
|
| 147 |
+
(2)
|
| 148 |
+
�
|
| 149 |
+
1 + z2
|
| 150 |
+
−z
|
| 151 |
+
−z − z5 − z9
|
| 152 |
+
1 + z10
|
| 153 |
+
�
|
| 154 |
+
�
|
| 155 |
+
1 + z2
|
| 156 |
+
0
|
| 157 |
+
−z3 − z7
|
| 158 |
+
1 + z10
|
| 159 |
+
�
|
| 160 |
+
18
|
| 161 |
+
10
|
| 162 |
+
(3)
|
| 163 |
+
�
|
| 164 |
+
1 + z2
|
| 165 |
+
−z
|
| 166 |
+
−z
|
| 167 |
+
1 + z2
|
| 168 |
+
�
|
| 169 |
+
�
|
| 170 |
+
1 + z2 − z
|
| 171 |
+
0
|
| 172 |
+
0
|
| 173 |
+
1 + z2 − z
|
| 174 |
+
�
|
| 175 |
+
3
|
| 176 |
+
3
|
| 177 |
+
(4)
|
| 178 |
+
�
|
| 179 |
+
1 + z2
|
| 180 |
+
−z
|
| 181 |
+
−z − z2
|
| 182 |
+
1 + z3
|
| 183 |
+
�
|
| 184 |
+
�
|
| 185 |
+
1 + z2 − z
|
| 186 |
+
0
|
| 187 |
+
0
|
| 188 |
+
1 + z3
|
| 189 |
+
�
|
| 190 |
+
5
|
| 191 |
+
3
|
| 192 |
+
(5)
|
| 193 |
+
�
|
| 194 |
+
1 + z2
|
| 195 |
+
−z
|
| 196 |
+
−z
|
| 197 |
+
1 + z2 − z
|
| 198 |
+
�
|
| 199 |
+
�
|
| 200 |
+
1 + z2
|
| 201 |
+
0
|
| 202 |
+
0
|
| 203 |
+
1 + z2
|
| 204 |
+
�
|
| 205 |
+
5
|
| 206 |
+
2
|
| 207 |
+
(6)
|
| 208 |
+
Table 1: Finite type classification for Y-systems of rank 2. The numbers h± are the length of
|
| 209 |
+
reddening sequences in positive and negative directions, respectively.
|
| 210 |
+
Theorem 1.5. Suppose that I = {1, 2}.
|
| 211 |
+
(1) Any pair A±(z) ∈ Y in Table 1 is of finite type.
|
| 212 |
+
(2) Any indecomposable pair A±(z) ∈ Y of finite type is reduced to exactly one pair in Table 1
|
| 213 |
+
by permuting the indices, changing sign, and changing slices (see Section 3.1), if necessary.
|
| 214 |
+
The claim (1) can be proved by concrete calculation in a suitable universal algebra since
|
| 215 |
+
A±(z) in Table 1 is concrete. We, however, give another proof involving cluster algebras. We
|
| 216 |
+
give a quiver and a sequence of mutations for each A±(z) in Table 1 that yields the Y-system as
|
| 217 |
+
the exchange relation of coefficients in the cluster algebra. See Table 3 for quivers and mutations.
|
| 218 |
+
We can verify that some iteration of this sequence of mutations, as well as its inverse, is a
|
| 219 |
+
reddening sequence (Theorem 2.8). Thanks to the deep results in the theory of cluster algebras,
|
| 220 |
+
this property is enough to imply the periodicity (Proposition 2.7). The number h± in Table
|
| 221 |
+
1 are the length of reddening sequences in positive and negative directions, respectively. This
|
| 222 |
+
verification of the periodicity is interesting not only because it is computationally more efficient,
|
| 223 |
+
but also because it leads to nontrivial dilogarithm identities associated with Donaldson-Thomas
|
| 224 |
+
invariants (Corollary 2.10).
|
| 225 |
+
The claim (2) is proved in Section 3.2 by the following steps:
|
| 226 |
+
Step 1. We recall the result in [24] that asserts that A±(1) satisfies a certain positivity, which
|
| 227 |
+
in particular implies that tr A±(1) and det A±(1) are positive. This allows us to significantly
|
| 228 |
+
reduce the candidates for finite type A±(z).
|
| 229 |
+
Step 2. For a fixed A+(1) in the candidates obtained in Step 1, we search for A−(1) satisfying
|
| 230 |
+
the symplectic property (1.4) at z = 1.
|
| 231 |
+
Step 3. During the search in Step 2, we discard the pair A±(1) that cannot be endowed with
|
| 232 |
+
the parameter z (Lemma 3.3 and 3.4).
|
| 233 |
+
Step 4. At this point, we have six candidates up to a permutation of the indices and a change of
|
| 234 |
+
sign. For each A±(1) in the six candidates, we try to endow with the parameter z. It turns out
|
| 235 |
+
that this is possible for all the six candidates. We give all possible A±(z) in Lemma 3.5–3.8.
|
| 236 |
+
3
|
| 237 |
+
|
| 238 |
+
Step 5. We finally check that each remaining candidate reduces to one of A±(z) in Table 1 by
|
| 239 |
+
change of slices.
|
| 240 |
+
Remark 1.6. Most of the Y-systems obtained from Table 1 are already known in the litera-
|
| 241 |
+
ture. (1)op and (6)op are Zamolodchikov’s Y-system of type A2 [36] and T2 (“tadpole”) [30],
|
| 242 |
+
respectively. (2)op is the reduced sine-Gordon Y-system associated with the continued fraction
|
| 243 |
+
3/4 = [1, 3] = 1/(1+ 1/3), and (5)op with z replaced by z2 is the reduced sine-Gordon Y-system
|
| 244 |
+
associated with 3/5 = [1, 1, 2] = 1/(1 + 1/(1 + 1/2)) [32] . (4) is the “half” of the Y-system
|
| 245 |
+
associated with the pair (A2, A2) [30]. (3) appears to be new:
|
| 246 |
+
Y1(u)Y1(u − 2) =
|
| 247 |
+
1
|
| 248 |
+
1 + Y2(u − 1)−1
|
| 249 |
+
Y2(u)Y2(u − 10) =
|
| 250 |
+
�
|
| 251 |
+
1 + Y1(u − 3)
|
| 252 |
+
��
|
| 253 |
+
1 + Y1(u − 7)
|
| 254 |
+
�
|
| 255 |
+
�
|
| 256 |
+
1 + Y1(u − 1)−1��
|
| 257 |
+
1 + Y1(u − 5)−1��
|
| 258 |
+
1 + Y1(u − 9)−1�
|
| 259 |
+
although it is implicitly given in the author’s previous work [24, Table 2].
|
| 260 |
+
Remark 1.7. The pair A±(z) ∈ Y is called the T-datum in [24] since it describes the T-systems,
|
| 261 |
+
which is a companion to the Y-systems. We do not use this term since we only consider the
|
| 262 |
+
Y-systems in this paper. Moreover, the definition of the T-datum in [24] allows to have a non-
|
| 263 |
+
diagonal N0 and have a nontrivial symmetrizer D, which is more general than the definition in
|
| 264 |
+
this paper. See also Section 1.4 for the Y-systems involving nontrivial symmetrizers.
|
| 265 |
+
Remark 1.8. There is another expression of the Y-system using a pair of matrices A±(z)
|
| 266 |
+
directly. Let A±(z) ∈ Y0, and define aij;p ∈ Z by
|
| 267 |
+
A±(z) =
|
| 268 |
+
��
|
| 269 |
+
p∈N
|
| 270 |
+
a±
|
| 271 |
+
ij;pzp
|
| 272 |
+
�
|
| 273 |
+
i,j∈I
|
| 274 |
+
.
|
| 275 |
+
Let (P ±
|
| 276 |
+
i (u))i∈I,u∈Z be a family of elements in a multiplicative abelian group P. We say that
|
| 277 |
+
(P ±
|
| 278 |
+
i (u)) satisfies the multiplicative Y-system associated with A±(z) if
|
| 279 |
+
�
|
| 280 |
+
j∈I
|
| 281 |
+
�
|
| 282 |
+
p∈N
|
| 283 |
+
P +
|
| 284 |
+
j (u − p)a+
|
| 285 |
+
ij;p =
|
| 286 |
+
�
|
| 287 |
+
j∈I
|
| 288 |
+
�
|
| 289 |
+
p∈N
|
| 290 |
+
P −
|
| 291 |
+
j (u − p)a−
|
| 292 |
+
ij;p
|
| 293 |
+
(1.5)
|
| 294 |
+
for any i, u (schematically, “A+(z) · log P + = A−(z) · log P −” under the action z : u �→ u − 1).
|
| 295 |
+
The solution (P ±
|
| 296 |
+
i (u)) is called normalized if P is endowed with a semifield structure, and
|
| 297 |
+
P +
|
| 298 |
+
i (u) + P −
|
| 299 |
+
i (u) = 1
|
| 300 |
+
for any i, u. We have a one-to-one correspondence between solutions of the Y-system (1.1) and
|
| 301 |
+
normalized solutions of the multiplicative Y-system (1.5). The correspondence is given by
|
| 302 |
+
Yi(u) �→ P +
|
| 303 |
+
i (u)
|
| 304 |
+
P −
|
| 305 |
+
i (u),
|
| 306 |
+
P +
|
| 307 |
+
i (u) �→
|
| 308 |
+
Yi(u)
|
| 309 |
+
1 + Yi(u),
|
| 310 |
+
P −
|
| 311 |
+
i (u) �→
|
| 312 |
+
1
|
| 313 |
+
1 + Yi(u).
|
| 314 |
+
In the setting of cluster algebras, this correspondence is nothing but the normalization of the
|
| 315 |
+
coefficients described by Fomin and Zelevinsky [7, Section 5].
|
| 316 |
+
1.3
|
| 317 |
+
Relation to Nahm sums
|
| 318 |
+
Consider the q-series defined by
|
| 319 |
+
G(q) =
|
| 320 |
+
∞
|
| 321 |
+
�
|
| 322 |
+
n=0
|
| 323 |
+
qn2
|
| 324 |
+
(q)n
|
| 325 |
+
,
|
| 326 |
+
H(q) =
|
| 327 |
+
∞
|
| 328 |
+
�
|
| 329 |
+
n=0
|
| 330 |
+
qn2+n
|
| 331 |
+
(q)n
|
| 332 |
+
,
|
| 333 |
+
(1.6)
|
| 334 |
+
4
|
| 335 |
+
|
| 336 |
+
where (q)n := (1 − q)(1 − q2) · · · (1 − qn) is the q-Pochhammer symbol. The famous Rogers-
|
| 337 |
+
Ramanujan identities express these q-series as the following infinite products:
|
| 338 |
+
G(q) =
|
| 339 |
+
�
|
| 340 |
+
n≡±1 mod 5
|
| 341 |
+
1
|
| 342 |
+
1 − qn,
|
| 343 |
+
H(q) =
|
| 344 |
+
�
|
| 345 |
+
n≡±2 mod 5
|
| 346 |
+
1
|
| 347 |
+
1 − qn.
|
| 348 |
+
These expressions in particular implies that q−1/60G(q) and q11/60H(q) are modular functions
|
| 349 |
+
on some finite index subgroup of SL(2, Z). In fact, it is a rare case that an infinite sum of the
|
| 350 |
+
form (1.6) is modular. It is known that the q-series
|
| 351 |
+
∞
|
| 352 |
+
�
|
| 353 |
+
n=0
|
| 354 |
+
q
|
| 355 |
+
1
|
| 356 |
+
2 an2+bn+c
|
| 357 |
+
(q)n
|
| 358 |
+
(1.7)
|
| 359 |
+
with a, b, c ∈ Q is modular only if a = 1/2, 1, or 2 [35].
|
| 360 |
+
Nahm [26] considered higher rank generalization of (1.7), which we call the Nahm sum. Let
|
| 361 |
+
I be a finite set, and suppose that A ∈ QI×I is a symmetric positive definite matrix, B ∈ QI is
|
| 362 |
+
a vector, and C ∈ Q is a scalar. The Nahm sum is the q-series defined by
|
| 363 |
+
fA,B,C(q) :=
|
| 364 |
+
�
|
| 365 |
+
n∈NI
|
| 366 |
+
q
|
| 367 |
+
1
|
| 368 |
+
2 nTAn+nTB+C
|
| 369 |
+
�
|
| 370 |
+
a(q)ni
|
| 371 |
+
.
|
| 372 |
+
When |I| ≥ 2, it is not well understood when fA,B,C(q) is modular. Nahm gave a conjecture
|
| 373 |
+
providing a criterion on the modularity of fA,B,C(q) in terms of torsion elements in the Bloch
|
| 374 |
+
group [26, 35]. See [3, 33] for the development of this conjecture.
|
| 375 |
+
Nahm used Zamolodchikov’s periodicity to provide an evidence of the conjecture. In fact,
|
| 376 |
+
there is a natural way to give a candidate of modular Nahm sums from finite type A±(z) ∈ Y
|
| 377 |
+
in general. Precisely, the matrix K := A+(1)−1A−(1) is always symmetric and positive definite
|
| 378 |
+
for finite type A±(z) ∈ Y, and it is conjectured that it gives a modular Nahm sum fK,0,C(q) for
|
| 379 |
+
some C [24]. (This construction is essentially the same as that in [18], except that they did not
|
| 380 |
+
prove that K is symmetric and positive definite. A special case can also be found in [23].) We
|
| 381 |
+
note that the symplectic property (1.4) at z = 1 plays an important role here since it implies
|
| 382 |
+
that K is symmetric. On the other hand, the positive definiteness is related to the periodicity
|
| 383 |
+
of the Y-system.
|
| 384 |
+
Based on our classification, we find that:
|
| 385 |
+
Theorem 1.9. Suppose that I = {1, 2}. The Nahm sum fK,0,C(q) is modular for any finite type
|
| 386 |
+
A±(z) ∈ Y, where C is given in Table 2.
|
| 387 |
+
In fact, every K from finite type A±(z) is included in the Zagier’s list [35, Table 2] for rank
|
| 388 |
+
2 candidates of modular Nahm sums. There are Rogers-Ramanujan type identities that enable
|
| 389 |
+
us to write each Nahm sum in the list in terms of theta functions. The proof of the desired
|
| 390 |
+
identities was partially given in [1, 4, 6, 33, 35], and was recently completed by Wang [34] except
|
| 391 |
+
for one candidate that does not appears in our construction from Y-systems. See Table 2.
|
| 392 |
+
Remark 1.10. We can define the refinement f (s)
|
| 393 |
+
A±(z)(q) of the Nahm sum fK,0,0(q), which is
|
| 394 |
+
parametrized by s ∈ H for an abelian group H of order det A+(1) such that it reduces to the
|
| 395 |
+
original one by taking summation [24, Definition 5.12]:
|
| 396 |
+
fK,0,0(q) =
|
| 397 |
+
�
|
| 398 |
+
s∈H
|
| 399 |
+
f (s)
|
| 400 |
+
A±(z)(q).
|
| 401 |
+
It is conjectured that each f (s)
|
| 402 |
+
A±(z)(q) is already modular after multiplying qC for some C. We
|
| 403 |
+
note that the symplectic property (1.4) at z = 1 again plays an important role in the definition
|
| 404 |
+
of the refinement. We will discuss this refinement for rank 2 case in more detail elsewhere. We
|
| 405 |
+
remark that similar refinement also appears in the context of 3-dimensional quantum topology
|
| 406 |
+
[13, Section 6.3].
|
| 407 |
+
5
|
| 408 |
+
|
| 409 |
+
A±(z)
|
| 410 |
+
K
|
| 411 |
+
−24C
|
| 412 |
+
RR
|
| 413 |
+
A±(z)
|
| 414 |
+
K
|
| 415 |
+
−24C
|
| 416 |
+
RR
|
| 417 |
+
(1)
|
| 418 |
+
�
|
| 419 |
+
4/3
|
| 420 |
+
2/3
|
| 421 |
+
2/3
|
| 422 |
+
4/3
|
| 423 |
+
�
|
| 424 |
+
4
|
| 425 |
+
5
|
| 426 |
+
[6]
|
| 427 |
+
(1)op
|
| 428 |
+
�
|
| 429 |
+
1
|
| 430 |
+
−1/2
|
| 431 |
+
−1/2
|
| 432 |
+
1
|
| 433 |
+
�
|
| 434 |
+
6
|
| 435 |
+
5
|
| 436 |
+
[33]
|
| 437 |
+
(2)
|
| 438 |
+
�3/2
|
| 439 |
+
1
|
| 440 |
+
1
|
| 441 |
+
2
|
| 442 |
+
�
|
| 443 |
+
5
|
| 444 |
+
7
|
| 445 |
+
[34]
|
| 446 |
+
(2)op
|
| 447 |
+
�
|
| 448 |
+
1
|
| 449 |
+
−1/2
|
| 450 |
+
−1/2
|
| 451 |
+
3/4
|
| 452 |
+
�
|
| 453 |
+
9
|
| 454 |
+
7
|
| 455 |
+
[34]
|
| 456 |
+
(3), (6)
|
| 457 |
+
�2
|
| 458 |
+
2
|
| 459 |
+
2
|
| 460 |
+
4
|
| 461 |
+
�
|
| 462 |
+
4
|
| 463 |
+
7
|
| 464 |
+
[1]
|
| 465 |
+
(3)op, (6)op
|
| 466 |
+
�
|
| 467 |
+
1
|
| 468 |
+
−1/2
|
| 469 |
+
−1/2
|
| 470 |
+
1/2
|
| 471 |
+
�
|
| 472 |
+
10
|
| 473 |
+
7
|
| 474 |
+
[34]
|
| 475 |
+
(4)
|
| 476 |
+
�
|
| 477 |
+
2/3
|
| 478 |
+
1/3
|
| 479 |
+
1/3
|
| 480 |
+
2/3
|
| 481 |
+
�
|
| 482 |
+
1
|
| 483 |
+
[35]
|
| 484 |
+
(4)op
|
| 485 |
+
� 2
|
| 486 |
+
−1
|
| 487 |
+
−1
|
| 488 |
+
2
|
| 489 |
+
�
|
| 490 |
+
1
|
| 491 |
+
[35]
|
| 492 |
+
(5)
|
| 493 |
+
�1
|
| 494 |
+
1
|
| 495 |
+
1
|
| 496 |
+
2
|
| 497 |
+
�
|
| 498 |
+
3
|
| 499 |
+
4
|
| 500 |
+
[34]
|
| 501 |
+
(5)op
|
| 502 |
+
� 2
|
| 503 |
+
−1
|
| 504 |
+
−1
|
| 505 |
+
1
|
| 506 |
+
�
|
| 507 |
+
5
|
| 508 |
+
4
|
| 509 |
+
[4]
|
| 510 |
+
Table 2: The list of the matrix K = A+(1)−1A−(1). The Nahm sum fK,0,C(q) is modular, which
|
| 511 |
+
can be proved by using Rogers-Ramanujan type identities (RR for short) given in the references
|
| 512 |
+
in the table.
|
| 513 |
+
1.4
|
| 514 |
+
Remarks on higher rank and skew-symmetrizable case
|
| 515 |
+
We have seen that the following properties hold for rank 2 case:
|
| 516 |
+
(P1) We have reddening sequences in both positive and negative directions.
|
| 517 |
+
(P2) The map A±(z) �→ A+(1)−1A−(1) gives modular Nahm sums.
|
| 518 |
+
We expect that the properties (P1) and (P2) also hold for any finite type A±(z) ∈ Y of general
|
| 519 |
+
rank. The followings are some known examples:
|
| 520 |
+
• For the Y-system associated with the untwisted quantum affine algebras Uq(X(1)
|
| 521 |
+
r ) with
|
| 522 |
+
level ℓ restriction [22], (P1) holds with h+ = tℓ and h− = t · (dual Coxeter number of Xr)
|
| 523 |
+
where t = 1, 2, or 3 is the multiplicity in the Dynkin diagram of Xr [15, 16], and (P2)
|
| 524 |
+
holds under the assumption [14, Conjecture 5.3] by the result of Kac and Peterson [17].
|
| 525 |
+
• For the Y-system associated with a pair of finite type simply laced Dynkin type (Xr, X′
|
| 526 |
+
r′)
|
| 527 |
+
[30], (P1) holds with h+ = (Coxeter number of Xr) and h− = (Coxeter number of X′
|
| 528 |
+
r′)
|
| 529 |
+
[19, 21].
|
| 530 |
+
• For the (reduced) sine-Gordon Y-system associated with the continued fraction p/q =
|
| 531 |
+
[nF, . . . , n1] = 1/(nF + 1/(· · · + 1/n1)) [29, 32], (P1) appears to hold with h+ = 2p and
|
| 532 |
+
h− = 2q.
|
| 533 |
+
• For the Y-system associated with an admissible ADE bigraph (Γ, ∆) [12], (P1) appears to
|
| 534 |
+
hold with h+ = (Coxeter number of Γ) and h− = (Coxeter number of ∆).
|
| 535 |
+
Moreover, we can consider Y-systems associated with skew-symmetrizable cluster algebras
|
| 536 |
+
rather than skew-symmetric ones discussed in this paper. In this case, the symplectic property
|
| 537 |
+
(1.4) becomes
|
| 538 |
+
A+(z)DA−(z−1)T = A−(z)DA+(z−1)T,
|
| 539 |
+
where D is a diagonal matrix called symmetrizer [24]. We also expect that the properties (P1)
|
| 540 |
+
and (P2) also hold for skew-symmetrizable case. See [24, Definition 5.12] for the definition of
|
| 541 |
+
the Nahm sum in skew-symmetrizable case.
|
| 542 |
+
Acknowledgment. This work is supported by JSPS KAKENHI Grant Number JP21J00050.
|
| 543 |
+
6
|
| 544 |
+
|
| 545 |
+
2
|
| 546 |
+
Y-systems and cluster algebras
|
| 547 |
+
2.1
|
| 548 |
+
Preliminaries on cluster algebras
|
| 549 |
+
In this paper, a semifield is a multiplicative abelian group equipped with an addition that is
|
| 550 |
+
commutative, associative, and distributive with respect to the multiplication.
|
| 551 |
+
Definition 2.1. Let I be a set.
|
| 552 |
+
The set of all nonzero rational functions in the variables
|
| 553 |
+
y = (yi)i∈I with natural number coefficients is a semifield with respect to the usual addition
|
| 554 |
+
and multiplication. This semifield is called the universal semifield, and denoted by Q>0(y). We
|
| 555 |
+
have a canonical bijection Homsemifield(Q>0(y), P) ∼= Homset(I, P) for any set I and semifield P.
|
| 556 |
+
Definition 2.2. Let I be a set. The tropical semifield Trop(y) is the multiplicative free abelian
|
| 557 |
+
group generated by the variables y = (yi)i∈I equipped with the addition defined by
|
| 558 |
+
�
|
| 559 |
+
i
|
| 560 |
+
yai
|
| 561 |
+
i +
|
| 562 |
+
�
|
| 563 |
+
i
|
| 564 |
+
ybi
|
| 565 |
+
i =
|
| 566 |
+
�
|
| 567 |
+
i
|
| 568 |
+
ymin(ai,bi)
|
| 569 |
+
i
|
| 570 |
+
.
|
| 571 |
+
Let I be a finite set and P be a semifield. A Y-seed is a pair (B, y) where B = (Bij)i,j∈I
|
| 572 |
+
is a skew-symmetric integer matrix and y = (yi)i∈I is a tuple of elements in P. We sometimes
|
| 573 |
+
represent B as the quiver whose signed adjacency matrix is B. For a Y-seed (B, y) and k ∈ I,
|
| 574 |
+
the mutation in direction k transforms (B, y) into the new Y-seed µk(B, y) = (B′, y′) given by
|
| 575 |
+
B′
|
| 576 |
+
ij :=
|
| 577 |
+
�
|
| 578 |
+
−Bij
|
| 579 |
+
if i = k or j = k,
|
| 580 |
+
Bij + [−Bik]+Bkj + Bik[Bkj]+
|
| 581 |
+
otherwise,
|
| 582 |
+
(2.1)
|
| 583 |
+
y′
|
| 584 |
+
i :=
|
| 585 |
+
�
|
| 586 |
+
yk
|
| 587 |
+
if i = k,
|
| 588 |
+
yiy[Bki]+
|
| 589 |
+
k
|
| 590 |
+
(1 + yk)−Bki
|
| 591 |
+
otherwise.
|
| 592 |
+
(2.2)
|
| 593 |
+
A mutation is involutive, that is, µk(B, y) = (B′, y′) implies (B, y) = µk(B′, y′). We have the
|
| 594 |
+
commutativity
|
| 595 |
+
µiµj = µjµi
|
| 596 |
+
if Bij = 0,
|
| 597 |
+
(2.3)
|
| 598 |
+
which allows us to write µi for a set i ⊆ I such that Bij = 0 for any i, j ∈ i to mean the
|
| 599 |
+
successive mutations along arbitrarily chosen order on i.
|
| 600 |
+
For a Y-seed (B, y) and a bijection ν : I → I, we define a new Y-seed ν(B, y) = (B′, y′) by
|
| 601 |
+
B′
|
| 602 |
+
ν(i)ν(j) := Bij and y′
|
| 603 |
+
ν(i) := yi.
|
| 604 |
+
2.2
|
| 605 |
+
Solving Y-systems by cluster algebras
|
| 606 |
+
Let A±(z) ∈ Y. We will construct a solution of the Y-system associated with A±(z) based on
|
| 607 |
+
[24, Section 3.3]. We first define a subset R ⊆ I × Z by
|
| 608 |
+
R := {(i, u) ∈ I × Z | 0 ≤ u < ri},
|
| 609 |
+
(2.4)
|
| 610 |
+
and define a skew-symmetric R × R integer matrix B by
|
| 611 |
+
B(i,p)(j,q) = −nij;p−q + nji;q−p +
|
| 612 |
+
�
|
| 613 |
+
k∈I
|
| 614 |
+
min(p,q)
|
| 615 |
+
�
|
| 616 |
+
v=0
|
| 617 |
+
�
|
| 618 |
+
n+
|
| 619 |
+
ik;p−vn−
|
| 620 |
+
jk;q−v − n−
|
| 621 |
+
ik;p−vn+
|
| 622 |
+
jk;q−v
|
| 623 |
+
�
|
| 624 |
+
,
|
| 625 |
+
(2.5)
|
| 626 |
+
where we understand nij;p = 0 if p < 0. We then define i := {(i, u) | u = 0} ⊆ R. We also define
|
| 627 |
+
a bijection ν : R → R by
|
| 628 |
+
ν(i, p) =
|
| 629 |
+
�
|
| 630 |
+
(i, p − 1)
|
| 631 |
+
if p > 0,
|
| 632 |
+
(i, ri)
|
| 633 |
+
if p = 0.
|
| 634 |
+
(2.6)
|
| 635 |
+
7
|
| 636 |
+
|
| 637 |
+
Then the symplectic property (1.4) ensures that ν(µi(B)) = B [24, Lemma 3.16]. We finally
|
| 638 |
+
define a sequence of Y-seeds
|
| 639 |
+
· · · → (B, y(−1)) → (B, y(0)) → (B, y(1)) → · · ·
|
| 640 |
+
(2.7)
|
| 641 |
+
in Q>0(y) by y(0) := y and (B, y(u + 1)) = ν(µi(B, y(u))). The sequence (2.7) gives a solution
|
| 642 |
+
of the Y-system:
|
| 643 |
+
Lemma 2.3. [24, Theorem 3.13] (yi,0(u))i∈I,u∈Z satisfies the Y-system associated with A±(z).
|
| 644 |
+
This solution is universal in the following sense.
|
| 645 |
+
Lemma 2.4. [24, Theorem 3.19] Suppose that a family (Yi(u))i∈I,u∈Z satisfies the Y-system
|
| 646 |
+
associated with A±(z). Define a semifield homomorphism f : Q>0(y) → P by
|
| 647 |
+
f(yi,p) := Yi(p)
|
| 648 |
+
�
|
| 649 |
+
j∈I
|
| 650 |
+
p
|
| 651 |
+
�
|
| 652 |
+
q=0
|
| 653 |
+
Yj(p − q)−[nij;q]+�
|
| 654 |
+
1 + Yj(p − q)
|
| 655 |
+
�nij;q.
|
| 656 |
+
(2.8)
|
| 657 |
+
Then f(yi,0(u)) = Yi(u) for any i, u.
|
| 658 |
+
Corollary 2.5. A±(z) ∈ Y is of finite type if and only if there are different integers u, v such
|
| 659 |
+
that y(u) = y(v) in (2.7).
|
| 660 |
+
2.3
|
| 661 |
+
Periodicity and reddening sequences
|
| 662 |
+
Similarly to (2.7), we define a sequence of Y-seeds
|
| 663 |
+
· · · → (B, y(−1)) → (B, y(0)) → (B, y(1)) → · · ·
|
| 664 |
+
(2.9)
|
| 665 |
+
by the same formulas but now in Trop(y) rather than Q(y).
|
| 666 |
+
Definition 2.6. We say that the Y-system associated with A±(z) ∈ Y is positive (resp. negative)
|
| 667 |
+
reddening if there is a positive integer u such that all the exponents in yi(u) (resp. yi(−u)) in
|
| 668 |
+
(2.9) are nonpositive for any i. We denote by h+ (resp. h−) the least such positive integer u.
|
| 669 |
+
Equivalently, the Y-system is positive (resp. negative) reddening if and only if all the en-
|
| 670 |
+
tries in the C-matrix associated with the sequence of mutations (B, y(0)) → (B, y(u)) (resp.
|
| 671 |
+
(B, y(0)) → (B, y(−u))) are nonpositive for some u > 0.
|
| 672 |
+
Proposition 2.7. Suppose that the Y-system associated with A±(z) is positive and negative
|
| 673 |
+
reddening. Then A±(z) is of finite type.
|
| 674 |
+
Proof. We verify the equivalent condition in Corollary 2.5. By [2, Proposition 2.10], there are
|
| 675 |
+
bijections σ, σ′ : R → R such that yi(h+) = y−1
|
| 676 |
+
σ(i) and yi(−h−) = y−1
|
| 677 |
+
σ′(i) for any i (in other
|
| 678 |
+
words, the C-matrices associated with them are the minus of permutation matrices). Now the
|
| 679 |
+
claim follows from the separation formula for y-variables [10, Proposition 3.13] and the result
|
| 680 |
+
on C-matrices shown by Cao, Huang, and Li [5, Theorem 2.5]. See also [28, Theorem 5.2] for
|
| 681 |
+
the corresponding statement dealing with permutations that is actually suitable here.
|
| 682 |
+
Theorem 2.8. The Y-system associated with each A±(z) in Table 1 is positive and negative
|
| 683 |
+
reddening.
|
| 684 |
+
Proof. The quiver B associated with A±(z) is given in Table 3. We can verify the assertion by
|
| 685 |
+
concrete calculation on the quiver. The numbers h± are given in Table 1.
|
| 686 |
+
8
|
| 687 |
+
|
| 688 |
+
Quiver B
|
| 689 |
+
A±(z)
|
| 690 |
+
(1, 0)
|
| 691 |
+
(2, 1)
|
| 692 |
+
(1, 1)
|
| 693 |
+
(2, 0)
|
| 694 |
+
(1)
|
| 695 |
+
(1, 0)
|
| 696 |
+
(2, 1)
|
| 697 |
+
(2, 3)
|
| 698 |
+
(2, 5)
|
| 699 |
+
(1, 1)
|
| 700 |
+
(2, 0)
|
| 701 |
+
(2, 2)
|
| 702 |
+
(2, 4)
|
| 703 |
+
(2)
|
| 704 |
+
(1, 0)
|
| 705 |
+
(2, 1)
|
| 706 |
+
(2, 3)
|
| 707 |
+
(2, 5)
|
| 708 |
+
(2, 7)
|
| 709 |
+
(2, 9)
|
| 710 |
+
(1, 1)
|
| 711 |
+
(2, 0)
|
| 712 |
+
(2, 2)
|
| 713 |
+
(2, 4)
|
| 714 |
+
(2, 6)
|
| 715 |
+
(2, 8)
|
| 716 |
+
(3)
|
| 717 |
+
(1, 0)
|
| 718 |
+
(2, 1)
|
| 719 |
+
(2, 0)
|
| 720 |
+
(1, 1)
|
| 721 |
+
(4)
|
| 722 |
+
(2, 0)
|
| 723 |
+
(1, 1)
|
| 724 |
+
(1, 0)
|
| 725 |
+
(2, 2)
|
| 726 |
+
(2, 1)
|
| 727 |
+
(5)
|
| 728 |
+
(1, 0)
|
| 729 |
+
(2, 1)
|
| 730 |
+
(2, 0)
|
| 731 |
+
(1, 1)
|
| 732 |
+
(6)
|
| 733 |
+
Table 3: Quivers associated with A±(z) in Table 1. Each quiver is preserved by the mutation at
|
| 734 |
+
(∗, 0) followed by the permutation (i, p) �→ (i, p − 1) (the second argument is considered modulo
|
| 735 |
+
ri), which yields Y-system. For (1)–(3), this operation interchanges the connected components
|
| 736 |
+
(see Section 3.1).
|
| 737 |
+
Theorem 1.5 (1) now follows from Proposition 2.7 and Theorem 2.8.
|
| 738 |
+
Remark 2.9. A connected component of each quiver in Table 3 has the following cluster type:
|
| 739 |
+
(1) A2
|
| 740 |
+
(2) A4
|
| 741 |
+
(3) E6
|
| 742 |
+
(4) D4
|
| 743 |
+
(5) A5
|
| 744 |
+
(6) A4
|
| 745 |
+
These are of finite type in the sense of [8], which also implies Theorem 1.5 (1). We remark,
|
| 746 |
+
however, that this observation is somewhat misleading since the quiver associated with a periodic
|
| 747 |
+
Y-system of general rank is typically of infinite type.
|
| 748 |
+
It might be better to think that the
|
| 749 |
+
appearance of only finite type quivers happens “by chance” due to the smallness of 2, the rank
|
| 750 |
+
of Y-systems considered in this paper.
|
| 751 |
+
Theorem 2.8 also gives quantum dilogarithm identifies associated with Donaldson-Thomas
|
| 752 |
+
invariants. For any reddening sequence i starting from a quiver B, we can define a quantity
|
| 753 |
+
E(i) by using the quantum dilogarithm. We refer to [20, Remark 6.6] as the definition. This
|
| 754 |
+
quantity coincides with Kontsevich-Soibelman’s refined Donaldson-Thomas invariant associated
|
| 755 |
+
with B [20, 25]. In particular, E(i) does not depend on i, which gives the quantum dilogarithm
|
| 756 |
+
identifies. In our case, we have:
|
| 757 |
+
9
|
| 758 |
+
|
| 759 |
+
Corollary 2.10. For each A±(z) in Table 1, we have
|
| 760 |
+
E(µh+) = E(µ−h−),
|
| 761 |
+
where µ := ν ◦ µi is the sequence of mutations (together with the permutation) (B, y(0)) →
|
| 762 |
+
(B, y(1)) in (2.7).
|
| 763 |
+
For example, the pair (1) in Table 1 yields the famous pentagon identity of the quantum
|
| 764 |
+
dilogarithm.
|
| 765 |
+
3
|
| 766 |
+
Classification
|
| 767 |
+
3.1
|
| 768 |
+
Change of slices
|
| 769 |
+
We need to introduce an appropriate equivalence relation on the set Y, which identifies essentially
|
| 770 |
+
the same Y-systems. Before we get into the definition, we will see a typical example. Consider
|
| 771 |
+
the following Y-system:
|
| 772 |
+
Y1(u)Y1(u − 2) = (1 + Y2(u − 1)−1)−1
|
| 773 |
+
Y2(u)Y2(u − 2) = (1 + Y1(u − 1)−1)−1
|
| 774 |
+
(3.1)
|
| 775 |
+
which corresponds to A±(z) ∈ Y given by (1) in Table 1. This system of equations are defined
|
| 776 |
+
on the set [1, 2] × Z, but actually can be defined on each component of the following disjoint
|
| 777 |
+
union:
|
| 778 |
+
[1, 2] × Z =
|
| 779 |
+
1�
|
| 780 |
+
k=0
|
| 781 |
+
{(i, u) | i − u ≡ k mod 2}.
|
| 782 |
+
We informally call the algebraic relation defined on each subset the slice of the whole Y-system.
|
| 783 |
+
If (Yi(u)) is a solution of the Y-system for i − u ≡ 0 mod 2, then (Yi(u + 1)) is a solution of the
|
| 784 |
+
Y-system for i − u ≡ 1 mod 2. Thus it is enough to consider only one slice when considering
|
| 785 |
+
solutions. Now we consider another Y-system:
|
| 786 |
+
Y ′
|
| 787 |
+
1(u)Y ′
|
| 788 |
+
1(u − 3) = (1 + Y ′
|
| 789 |
+
2(u − 2)−1)−1
|
| 790 |
+
Y ′
|
| 791 |
+
2(u)Y ′
|
| 792 |
+
2(u − 3) = (1 + Y ′
|
| 793 |
+
1(u − 1)−1)−1.
|
| 794 |
+
(3.2)
|
| 795 |
+
which corresponds to A′
|
| 796 |
+
±(z) ∈ Y given by
|
| 797 |
+
A′
|
| 798 |
+
+(z) :=
|
| 799 |
+
�
|
| 800 |
+
1 + z3
|
| 801 |
+
−z2
|
| 802 |
+
−z
|
| 803 |
+
1 + z3
|
| 804 |
+
�
|
| 805 |
+
,
|
| 806 |
+
A′
|
| 807 |
+
−(z) :=
|
| 808 |
+
�
|
| 809 |
+
1 + z3
|
| 810 |
+
0
|
| 811 |
+
0
|
| 812 |
+
1 + z3
|
| 813 |
+
�
|
| 814 |
+
.
|
| 815 |
+
The Y-system (3.2) is decomposed into three slices:
|
| 816 |
+
[1, 2] × Z =
|
| 817 |
+
2�
|
| 818 |
+
k=0
|
| 819 |
+
{(i, u) | i − u ≡ k mod 3}.
|
| 820 |
+
We see that for any solution of (3.1) for i − u ≡ 0 mod 2,
|
| 821 |
+
Y ′
|
| 822 |
+
1(u) := Y1
|
| 823 |
+
�2
|
| 824 |
+
3u − 1
|
| 825 |
+
3
|
| 826 |
+
�
|
| 827 |
+
,
|
| 828 |
+
Y ′
|
| 829 |
+
2(u) := Y2
|
| 830 |
+
�2
|
| 831 |
+
3u
|
| 832 |
+
�
|
| 833 |
+
is a solution of (3.2) for i − u ≡ 2 mod 3. We also obtain solutions for the other two slices by
|
| 834 |
+
shifting u. Conversely, any solution of (3.1) is obtained from a solution of (3.2). Therefore, it
|
| 835 |
+
10
|
| 836 |
+
|
| 837 |
+
is enough to consider one of the Y-systems (3.1) and (3.2). In particular, A±(z) is of finite type
|
| 838 |
+
if and only if A′
|
| 839 |
+
±(z) is.
|
| 840 |
+
Now we work in the general setting. The idea is that each slice corresponds to each connected
|
| 841 |
+
component of the quiver associated with the matrix B defined by (2.5). Let A±(z) ∈ Y, and
|
| 842 |
+
assume that it is indecomposable. By [24, Proposition 3.24], we have a decomposition of the
|
| 843 |
+
matrix B and its index set R:
|
| 844 |
+
B =
|
| 845 |
+
t−1
|
| 846 |
+
�
|
| 847 |
+
u=0
|
| 848 |
+
B(u),
|
| 849 |
+
R =
|
| 850 |
+
t−1
|
| 851 |
+
�
|
| 852 |
+
u=0
|
| 853 |
+
R(u)
|
| 854 |
+
such that each B(u) is indecomposable and we have a cyclic sequence of mutations
|
| 855 |
+
B(0)
|
| 856 |
+
ν|R(0)◦µi(0)
|
| 857 |
+
−−−−−−−→ B(1) −→ · · · −→ B(t − 1)
|
| 858 |
+
ν|R(t−1)◦µi(t−1)
|
| 859 |
+
−−−−−−−−−−→ B(0)
|
| 860 |
+
(3.3)
|
| 861 |
+
where i(u) := i ∩ R(u). We say that two pairs A±(z) and A′
|
| 862 |
+
±(z) are related by change of slices
|
| 863 |
+
if they yield the same cyclic sequence (3.3) up to a change of indices and the commutativity of
|
| 864 |
+
mutations (2.3). (This commutativity is already implicitly used to justify the notation µi(u) as
|
| 865 |
+
stated below (2.3).)
|
| 866 |
+
Example 3.1. The pairs A±(z) and A′
|
| 867 |
+
±(z) associated with (3.1) and (3.2), respectively, are
|
| 868 |
+
related by change of slices. Indeed, we see that the sequence (3.3) for (3.1) is
|
| 869 |
+
(1, 0)
|
| 870 |
+
(2, 1)
|
| 871 |
+
ν◦µ(0,0)
|
| 872 |
+
−−−−−→ (1, 1)
|
| 873 |
+
(2, 0)
|
| 874 |
+
ν◦µ(1,0)
|
| 875 |
+
−−−−−→ (1, 0)
|
| 876 |
+
(2, 1) ,
|
| 877 |
+
whereas the sequence (3.3) for (3.2) is
|
| 878 |
+
(1, 0)
|
| 879 |
+
(2, 1)
|
| 880 |
+
ν′◦µ(0,0)
|
| 881 |
+
−−−−−→ (1, 2)
|
| 882 |
+
(2, 0)
|
| 883 |
+
ν′◦µ(1,0)
|
| 884 |
+
−−−−−→ (1, 1)
|
| 885 |
+
(2, 2)
|
| 886 |
+
ν′
|
| 887 |
+
−→ (1, 0)
|
| 888 |
+
(2, 1) .
|
| 889 |
+
These are the same sequence up to a change of indices.
|
| 890 |
+
3.2
|
| 891 |
+
Proof of the classification
|
| 892 |
+
In this section, we will prove Theorem 1.5 (2). We first recall the following result.
|
| 893 |
+
Lemma 3.2 ([24, Theorem 5.5]). Let A±(z) ∈ Y. Assume that A±(z) is of finite type. Then
|
| 894 |
+
there is a vector v ∈ RI such that v > 0, vA+(1) > 0, and vA−(1) > 0.
|
| 895 |
+
In particular,
|
| 896 |
+
tr A±(1) > 0 and det A±(1) > 0.
|
| 897 |
+
By Lemma 3.2, A+(1) and A−(1) are equal to one of the following matrices:
|
| 898 |
+
� 2
|
| 899 |
+
−1
|
| 900 |
+
−1
|
| 901 |
+
2
|
| 902 |
+
�
|
| 903 |
+
,
|
| 904 |
+
� 2
|
| 905 |
+
−1
|
| 906 |
+
−2
|
| 907 |
+
2
|
| 908 |
+
�
|
| 909 |
+
,
|
| 910 |
+
� 2
|
| 911 |
+
−1
|
| 912 |
+
−3
|
| 913 |
+
2
|
| 914 |
+
�
|
| 915 |
+
,
|
| 916 |
+
� 2
|
| 917 |
+
−1
|
| 918 |
+
−1
|
| 919 |
+
1
|
| 920 |
+
�
|
| 921 |
+
,
|
| 922 |
+
� 2
|
| 923 |
+
0
|
| 924 |
+
−n
|
| 925 |
+
2
|
| 926 |
+
�
|
| 927 |
+
,
|
| 928 |
+
� 2
|
| 929 |
+
0
|
| 930 |
+
−n
|
| 931 |
+
1
|
| 932 |
+
�
|
| 933 |
+
,
|
| 934 |
+
� 1
|
| 935 |
+
0
|
| 936 |
+
−n
|
| 937 |
+
1
|
| 938 |
+
�
|
| 939 |
+
up to a permutation of the indices. We give several lemmas about impossible pairs. Before
|
| 940 |
+
giving lemmas, we note that
|
| 941 |
+
n+
|
| 942 |
+
ij;p = 0
|
| 943 |
+
or
|
| 944 |
+
n−
|
| 945 |
+
ij;p = 0
|
| 946 |
+
(3.4)
|
| 947 |
+
for any i, j, p.
|
| 948 |
+
Lemma 3.3. It is impossible that A±(z) ∈ Y has the following forms:
|
| 949 |
+
(1) A+(1) =
|
| 950 |
+
�2
|
| 951 |
+
−a
|
| 952 |
+
∗
|
| 953 |
+
∗
|
| 954 |
+
�
|
| 955 |
+
, A−(1) =
|
| 956 |
+
�2
|
| 957 |
+
−b
|
| 958 |
+
∗
|
| 959 |
+
∗
|
| 960 |
+
�
|
| 961 |
+
for odd a, b.
|
| 962 |
+
11
|
| 963 |
+
|
| 964 |
+
(2) A+(1) =
|
| 965 |
+
�2
|
| 966 |
+
−a
|
| 967 |
+
∗
|
| 968 |
+
∗
|
| 969 |
+
�
|
| 970 |
+
, A−(1) =
|
| 971 |
+
�1
|
| 972 |
+
−b
|
| 973 |
+
∗
|
| 974 |
+
∗
|
| 975 |
+
�
|
| 976 |
+
for odd a, b.
|
| 977 |
+
(3) A+(1) =
|
| 978 |
+
�1
|
| 979 |
+
−1
|
| 980 |
+
∗
|
| 981 |
+
∗
|
| 982 |
+
�
|
| 983 |
+
, A−(1) =
|
| 984 |
+
�1
|
| 985 |
+
−1
|
| 986 |
+
∗
|
| 987 |
+
∗
|
| 988 |
+
�
|
| 989 |
+
.
|
| 990 |
+
(4) A+(1) =
|
| 991 |
+
�1
|
| 992 |
+
0
|
| 993 |
+
∗
|
| 994 |
+
∗
|
| 995 |
+
�
|
| 996 |
+
, A−(1) =
|
| 997 |
+
�1
|
| 998 |
+
∗
|
| 999 |
+
∗
|
| 1000 |
+
∗
|
| 1001 |
+
�
|
| 1002 |
+
.
|
| 1003 |
+
Proof. For (2), we can set
|
| 1004 |
+
A+(z) =
|
| 1005 |
+
�1 + zr
|
| 1006 |
+
−f(z)
|
| 1007 |
+
∗
|
| 1008 |
+
∗
|
| 1009 |
+
�
|
| 1010 |
+
,
|
| 1011 |
+
A−(z) =
|
| 1012 |
+
�1 + zr − za
|
| 1013 |
+
−g(z)
|
| 1014 |
+
∗
|
| 1015 |
+
∗
|
| 1016 |
+
�
|
| 1017 |
+
.
|
| 1018 |
+
By the symplectic property (1.4), we have
|
| 1019 |
+
za + za−r + f(z)g(z−1) = z−a + zr−a + g(z)f(z−1).
|
| 1020 |
+
(3.5)
|
| 1021 |
+
Since 0 < a and a − r < 0 by (1.2), the sum of the coefficients of the terms in f(z)g(z−1)
|
| 1022 |
+
with positive exponents is equal to that with negative exponents. Since f(1)g(1) (=ab) is odd,
|
| 1023 |
+
f(z)g(z−1) should contain the constant term z0, which contradicts (3.4). The proof for (1) is
|
| 1024 |
+
similar.
|
| 1025 |
+
For (3), we can set
|
| 1026 |
+
A+(z) =
|
| 1027 |
+
���
|
| 1028 |
+
1 + zr − za
|
| 1029 |
+
−zb
|
| 1030 |
+
∗
|
| 1031 |
+
∗
|
| 1032 |
+
�
|
| 1033 |
+
,
|
| 1034 |
+
A−(z) =
|
| 1035 |
+
�
|
| 1036 |
+
1 + zr − zc
|
| 1037 |
+
−zd
|
| 1038 |
+
∗
|
| 1039 |
+
∗
|
| 1040 |
+
�
|
| 1041 |
+
with 0 < a, b, c, d < r. Without loss of generality, we can assume a < c. By (1.4), we have
|
| 1042 |
+
z−c + zr−c + za + za−r + zc−a + zd−b = zc + zc−r + z−a + zr−a + za−c + zb−d
|
| 1043 |
+
Since c − a > 0, we see that c − a is equal to c, r − a, or b − d. However, the first two cases are
|
| 1044 |
+
impossible by (1.2). Thus c − a = b − d, which implies that
|
| 1045 |
+
z−c + zr−c + za + za−r = zc + zc−r + z−a + zr−a.
|
| 1046 |
+
Since a > 0, we see that a is equal to c or r − a. However, a = c is impossible by (3.4). Thus
|
| 1047 |
+
a = r − a, which implies that
|
| 1048 |
+
z−c + zr−c = zc + zc−r.
|
| 1049 |
+
Since c > 0, we see that c = r − c. However, this implies that a = r/2 = c, which is impossible
|
| 1050 |
+
by (3.4).
|
| 1051 |
+
For (4), we can set
|
| 1052 |
+
A+(z) =
|
| 1053 |
+
�1 + zr − za
|
| 1054 |
+
0
|
| 1055 |
+
∗
|
| 1056 |
+
∗
|
| 1057 |
+
�
|
| 1058 |
+
,
|
| 1059 |
+
A−(z) =
|
| 1060 |
+
�
|
| 1061 |
+
1 + zr − zb
|
| 1062 |
+
∗
|
| 1063 |
+
∗
|
| 1064 |
+
∗
|
| 1065 |
+
�
|
| 1066 |
+
.
|
| 1067 |
+
By (1.4), we have
|
| 1068 |
+
za + za−r + z−b + zr−b + zb−a = z−a + zr−a + zb + zb−r + za−b.
|
| 1069 |
+
Comparing the number of the terms with positive and negative exponents, we should have a = b.
|
| 1070 |
+
This is impossible by (3.4).
|
| 1071 |
+
12
|
| 1072 |
+
|
| 1073 |
+
Lemma 3.4. It is impossible that indecomposable A±(z) ∈ Y has the form
|
| 1074 |
+
A+(1) =
|
| 1075 |
+
�∗
|
| 1076 |
+
0
|
| 1077 |
+
∗
|
| 1078 |
+
∗
|
| 1079 |
+
�
|
| 1080 |
+
,
|
| 1081 |
+
A−(1) =
|
| 1082 |
+
�∗
|
| 1083 |
+
0
|
| 1084 |
+
∗
|
| 1085 |
+
∗
|
| 1086 |
+
�
|
| 1087 |
+
.
|
| 1088 |
+
Proof. We can set
|
| 1089 |
+
A±(z) =
|
| 1090 |
+
�
|
| 1091 |
+
1 + zr1 − f±(z)
|
| 1092 |
+
0
|
| 1093 |
+
−g±(z)
|
| 1094 |
+
1 + zr2 − h±(z)
|
| 1095 |
+
�
|
| 1096 |
+
.
|
| 1097 |
+
Since g+(z) ̸= 0 or g−(z) ̸= 0, we can pick the least integer c among the exponents in g+(z) and
|
| 1098 |
+
g−(z). Without loss of generality, we can assume g+(1) contains the term zc. By (1.4), we have
|
| 1099 |
+
f+(z)g−(z−1) + (1 + zr1)g+(z−1) = f−(z)g+(z−1) + (1 + zr1)g−(z−1).
|
| 1100 |
+
(3.6)
|
| 1101 |
+
The left-hand side in (3.6) contains the term zr1−c, but any exponent in the right-hand side is
|
| 1102 |
+
strictly smaller that r1 − c by (1.2) and (3.4), which is a contradiction.
|
| 1103 |
+
We now search for possible pairs A±(1) case by case using the symplectic property (1.4) at
|
| 1104 |
+
z = 1 together with Lemma 3.3 and 3.4:
|
| 1105 |
+
• Case: A+(1) =
|
| 1106 |
+
� 2
|
| 1107 |
+
−1
|
| 1108 |
+
−1
|
| 1109 |
+
2
|
| 1110 |
+
�
|
| 1111 |
+
. The possibilities for A−(1) are:
|
| 1112 |
+
�2
|
| 1113 |
+
0
|
| 1114 |
+
0
|
| 1115 |
+
2
|
| 1116 |
+
�
|
| 1117 |
+
,
|
| 1118 |
+
�1
|
| 1119 |
+
0
|
| 1120 |
+
0
|
| 1121 |
+
1
|
| 1122 |
+
�
|
| 1123 |
+
.
|
| 1124 |
+
• Case: A+(1) =
|
| 1125 |
+
� 2
|
| 1126 |
+
−1
|
| 1127 |
+
−1
|
| 1128 |
+
2
|
| 1129 |
+
�
|
| 1130 |
+
. The possibilities for A−(1) are:
|
| 1131 |
+
�2
|
| 1132 |
+
0
|
| 1133 |
+
0
|
| 1134 |
+
2
|
| 1135 |
+
�
|
| 1136 |
+
,
|
| 1137 |
+
�1
|
| 1138 |
+
0
|
| 1139 |
+
0
|
| 1140 |
+
1
|
| 1141 |
+
�
|
| 1142 |
+
.
|
| 1143 |
+
• Case: A+(1) =
|
| 1144 |
+
� 2
|
| 1145 |
+
−1
|
| 1146 |
+
−2
|
| 1147 |
+
2
|
| 1148 |
+
�
|
| 1149 |
+
. The possibilities for A−(1) are:
|
| 1150 |
+
� 2
|
| 1151 |
+
0
|
| 1152 |
+
−1
|
| 1153 |
+
2
|
| 1154 |
+
�
|
| 1155 |
+
,
|
| 1156 |
+
�1
|
| 1157 |
+
0
|
| 1158 |
+
0
|
| 1159 |
+
2
|
| 1160 |
+
�
|
| 1161 |
+
.
|
| 1162 |
+
• Case: A+(1) =
|
| 1163 |
+
� 2
|
| 1164 |
+
−1
|
| 1165 |
+
−3
|
| 1166 |
+
2
|
| 1167 |
+
�
|
| 1168 |
+
. The possibilities for A−(1) are:
|
| 1169 |
+
� 2
|
| 1170 |
+
0
|
| 1171 |
+
−2
|
| 1172 |
+
2
|
| 1173 |
+
�
|
| 1174 |
+
.
|
| 1175 |
+
• Case: A+(1) =
|
| 1176 |
+
� 2
|
| 1177 |
+
−1
|
| 1178 |
+
−1
|
| 1179 |
+
1
|
| 1180 |
+
�
|
| 1181 |
+
. The possibilities for A−(1) are:
|
| 1182 |
+
�2
|
| 1183 |
+
0
|
| 1184 |
+
0
|
| 1185 |
+
2
|
| 1186 |
+
�
|
| 1187 |
+
,
|
| 1188 |
+
�1
|
| 1189 |
+
0
|
| 1190 |
+
0
|
| 1191 |
+
1
|
| 1192 |
+
�
|
| 1193 |
+
.
|
| 1194 |
+
13
|
| 1195 |
+
|
| 1196 |
+
• Case: A+(1) =
|
| 1197 |
+
� 2
|
| 1198 |
+
0
|
| 1199 |
+
−n
|
| 1200 |
+
2
|
| 1201 |
+
�
|
| 1202 |
+
. The possibilities for A±(1) are:
|
| 1203 |
+
��2
|
| 1204 |
+
0
|
| 1205 |
+
0
|
| 1206 |
+
2
|
| 1207 |
+
�
|
| 1208 |
+
,
|
| 1209 |
+
� 2
|
| 1210 |
+
−1
|
| 1211 |
+
−1
|
| 1212 |
+
2
|
| 1213 |
+
��
|
| 1214 |
+
,
|
| 1215 |
+
�� 2
|
| 1216 |
+
0
|
| 1217 |
+
−1
|
| 1218 |
+
2
|
| 1219 |
+
�
|
| 1220 |
+
,
|
| 1221 |
+
� 2
|
| 1222 |
+
−1
|
| 1223 |
+
−2
|
| 1224 |
+
2
|
| 1225 |
+
��
|
| 1226 |
+
,
|
| 1227 |
+
��2
|
| 1228 |
+
0
|
| 1229 |
+
0
|
| 1230 |
+
2
|
| 1231 |
+
�
|
| 1232 |
+
,
|
| 1233 |
+
� 1
|
| 1234 |
+
−1
|
| 1235 |
+
−1
|
| 1236 |
+
2
|
| 1237 |
+
��
|
| 1238 |
+
.
|
| 1239 |
+
• Case: A+(1) =
|
| 1240 |
+
� 2
|
| 1241 |
+
0
|
| 1242 |
+
−n
|
| 1243 |
+
1
|
| 1244 |
+
�
|
| 1245 |
+
. The possibilities for A±(1) are:
|
| 1246 |
+
��2
|
| 1247 |
+
0
|
| 1248 |
+
0
|
| 1249 |
+
1
|
| 1250 |
+
�
|
| 1251 |
+
,
|
| 1252 |
+
� 2
|
| 1253 |
+
−2
|
| 1254 |
+
−1
|
| 1255 |
+
2
|
| 1256 |
+
��
|
| 1257 |
+
.
|
| 1258 |
+
• Case: A+(1) =
|
| 1259 |
+
� 1
|
| 1260 |
+
0
|
| 1261 |
+
−n
|
| 1262 |
+
1
|
| 1263 |
+
�
|
| 1264 |
+
. The possibilities for A±(1) are:
|
| 1265 |
+
��2
|
| 1266 |
+
0
|
| 1267 |
+
0
|
| 1268 |
+
1
|
| 1269 |
+
�
|
| 1270 |
+
,
|
| 1271 |
+
� 2
|
| 1272 |
+
−2
|
| 1273 |
+
−1
|
| 1274 |
+
2
|
| 1275 |
+
��
|
| 1276 |
+
.
|
| 1277 |
+
In summary, the remaining possible pairs, up to a permutation of the indices and an change
|
| 1278 |
+
of sign, are given in the following table:
|
| 1279 |
+
A+(1)
|
| 1280 |
+
A−(1)
|
| 1281 |
+
� 2
|
| 1282 |
+
−1
|
| 1283 |
+
−1
|
| 1284 |
+
2
|
| 1285 |
+
�
|
| 1286 |
+
�2
|
| 1287 |
+
0
|
| 1288 |
+
0
|
| 1289 |
+
2
|
| 1290 |
+
�
|
| 1291 |
+
� 2
|
| 1292 |
+
−1
|
| 1293 |
+
−2
|
| 1294 |
+
2
|
| 1295 |
+
�
|
| 1296 |
+
� 2
|
| 1297 |
+
0
|
| 1298 |
+
−1
|
| 1299 |
+
2
|
| 1300 |
+
�
|
| 1301 |
+
� 2
|
| 1302 |
+
−1
|
| 1303 |
+
−3
|
| 1304 |
+
2
|
| 1305 |
+
�
|
| 1306 |
+
� 2
|
| 1307 |
+
0
|
| 1308 |
+
−2
|
| 1309 |
+
2
|
| 1310 |
+
�
|
| 1311 |
+
A+(1)
|
| 1312 |
+
A−(1)
|
| 1313 |
+
� 2
|
| 1314 |
+
−1
|
| 1315 |
+
−1
|
| 1316 |
+
2
|
| 1317 |
+
�
|
| 1318 |
+
�2
|
| 1319 |
+
0
|
| 1320 |
+
0
|
| 1321 |
+
2
|
| 1322 |
+
�
|
| 1323 |
+
� 2
|
| 1324 |
+
−1
|
| 1325 |
+
−2
|
| 1326 |
+
2
|
| 1327 |
+
�
|
| 1328 |
+
� 2
|
| 1329 |
+
0
|
| 1330 |
+
−1
|
| 1331 |
+
2
|
| 1332 |
+
�
|
| 1333 |
+
� 2
|
| 1334 |
+
−1
|
| 1335 |
+
−3
|
| 1336 |
+
2
|
| 1337 |
+
�
|
| 1338 |
+
� 2
|
| 1339 |
+
0
|
| 1340 |
+
−2
|
| 1341 |
+
2
|
| 1342 |
+
�
|
| 1343 |
+
(3.7)
|
| 1344 |
+
We now start searching for possible A±(z).
|
| 1345 |
+
Lemma 3.5. Let n ≥ 1. Suppose that
|
| 1346 |
+
A+(1) =
|
| 1347 |
+
� 2
|
| 1348 |
+
−1
|
| 1349 |
+
−n
|
| 1350 |
+
2
|
| 1351 |
+
�
|
| 1352 |
+
,
|
| 1353 |
+
A−(1) =
|
| 1354 |
+
�
|
| 1355 |
+
2
|
| 1356 |
+
0
|
| 1357 |
+
−(n − 1)
|
| 1358 |
+
2
|
| 1359 |
+
�
|
| 1360 |
+
.
|
| 1361 |
+
Then
|
| 1362 |
+
A+(z) =
|
| 1363 |
+
�
|
| 1364 |
+
[2]r
|
| 1365 |
+
−z−a
|
| 1366 |
+
−zr−a[n]2r
|
| 1367 |
+
[2](2n−1)r
|
| 1368 |
+
�
|
| 1369 |
+
,
|
| 1370 |
+
A−(z) =
|
| 1371 |
+
�
|
| 1372 |
+
[2]r
|
| 1373 |
+
0
|
| 1374 |
+
−z2r−a[n − 1]2r
|
| 1375 |
+
[2](2n−1)r
|
| 1376 |
+
�
|
| 1377 |
+
for some r, a, where [n]r is the z-integer defined by
|
| 1378 |
+
[n]r := 1 − zrn
|
| 1379 |
+
1 − zr .
|
| 1380 |
+
(3.8)
|
| 1381 |
+
Proof. We can set
|
| 1382 |
+
A+(z) =
|
| 1383 |
+
�
|
| 1384 |
+
[2]r1
|
| 1385 |
+
−za
|
| 1386 |
+
− �n
|
| 1387 |
+
i=1 zbi
|
| 1388 |
+
[2]r2
|
| 1389 |
+
�
|
| 1390 |
+
,
|
| 1391 |
+
A−(z) =
|
| 1392 |
+
�
|
| 1393 |
+
[2]r1
|
| 1394 |
+
0
|
| 1395 |
+
− �n−1
|
| 1396 |
+
i=1 zci
|
| 1397 |
+
[2]r2
|
| 1398 |
+
�
|
| 1399 |
+
.
|
| 1400 |
+
14
|
| 1401 |
+
|
| 1402 |
+
Without loss of generality, we can assume that
|
| 1403 |
+
b1 ≤ b2 ≤ · · · ≤ bn,
|
| 1404 |
+
c1 ≤ c2 ≤ · · · ≤ cn−1.
|
| 1405 |
+
By the symplectic property (1.4), we have
|
| 1406 |
+
n−1
|
| 1407 |
+
�
|
| 1408 |
+
i=1
|
| 1409 |
+
(z−ci + zr1−ci) + za + za−r2 =
|
| 1410 |
+
n
|
| 1411 |
+
�
|
| 1412 |
+
i=1
|
| 1413 |
+
(z−bi + zr1−bi).
|
| 1414 |
+
Comparing the degree by using the conditions (1.2) and (3.4), we obtain the system of linear
|
| 1415 |
+
equations
|
| 1416 |
+
a = r1 − b1,
|
| 1417 |
+
a − r2 = −bn,
|
| 1418 |
+
r1 = ci − bi = bi+1 − ci
|
| 1419 |
+
(i = 1, . . . , n − 1),
|
| 1420 |
+
which implies that
|
| 1421 |
+
r2 = (2n − 1)r1,
|
| 1422 |
+
bi = (2i − 1)r1 − a,
|
| 1423 |
+
ci = 2ir1 − a.
|
| 1424 |
+
Lemma 3.6. Suppose that
|
| 1425 |
+
A+(1) =
|
| 1426 |
+
� 2
|
| 1427 |
+
−1
|
| 1428 |
+
−1
|
| 1429 |
+
2
|
| 1430 |
+
�
|
| 1431 |
+
,
|
| 1432 |
+
A−(1) =
|
| 1433 |
+
�1
|
| 1434 |
+
0
|
| 1435 |
+
0
|
| 1436 |
+
1
|
| 1437 |
+
�
|
| 1438 |
+
.
|
| 1439 |
+
Then
|
| 1440 |
+
A+(z) =
|
| 1441 |
+
�
|
| 1442 |
+
1 + z2r
|
| 1443 |
+
−za
|
| 1444 |
+
−z2r−a
|
| 1445 |
+
1 + z2r
|
| 1446 |
+
�
|
| 1447 |
+
,
|
| 1448 |
+
A−(z) =
|
| 1449 |
+
�
|
| 1450 |
+
1 + z2r − zr
|
| 1451 |
+
0
|
| 1452 |
+
0
|
| 1453 |
+
1 + z2r − zr
|
| 1454 |
+
�
|
| 1455 |
+
for some r, a.
|
| 1456 |
+
Proof. We can set
|
| 1457 |
+
A+(z) =
|
| 1458 |
+
�
|
| 1459 |
+
1 + zr1
|
| 1460 |
+
−za
|
| 1461 |
+
−zb
|
| 1462 |
+
1 + zr2
|
| 1463 |
+
�
|
| 1464 |
+
,
|
| 1465 |
+
A−(z) =
|
| 1466 |
+
�
|
| 1467 |
+
1 + zr1 − zc
|
| 1468 |
+
0
|
| 1469 |
+
0
|
| 1470 |
+
1 + zr2 − zd
|
| 1471 |
+
�
|
| 1472 |
+
.
|
| 1473 |
+
By (1.4), we have r1 = r2 = a + b = 2c = 2d.
|
| 1474 |
+
Lemma 3.7. Suppose that
|
| 1475 |
+
A+(1) =
|
| 1476 |
+
� 2
|
| 1477 |
+
−1
|
| 1478 |
+
−2
|
| 1479 |
+
2
|
| 1480 |
+
�
|
| 1481 |
+
,
|
| 1482 |
+
A−(1) =
|
| 1483 |
+
�1
|
| 1484 |
+
0
|
| 1485 |
+
0
|
| 1486 |
+
2
|
| 1487 |
+
�
|
| 1488 |
+
.
|
| 1489 |
+
Then
|
| 1490 |
+
A+(z) =
|
| 1491 |
+
�
|
| 1492 |
+
1 + z2r
|
| 1493 |
+
−za
|
| 1494 |
+
−z2r−a − z3r−a
|
| 1495 |
+
1 + z3r
|
| 1496 |
+
�
|
| 1497 |
+
,
|
| 1498 |
+
A−(z) =
|
| 1499 |
+
�
|
| 1500 |
+
1 + z2r − zr
|
| 1501 |
+
0
|
| 1502 |
+
0
|
| 1503 |
+
1 + z2r
|
| 1504 |
+
�
|
| 1505 |
+
for some r, a.
|
| 1506 |
+
Proof. We can set
|
| 1507 |
+
A+(z) =
|
| 1508 |
+
�
|
| 1509 |
+
1 + zr1
|
| 1510 |
+
−za
|
| 1511 |
+
−zb1 − zb2
|
| 1512 |
+
1 + zr2
|
| 1513 |
+
�
|
| 1514 |
+
,
|
| 1515 |
+
A−(z) =
|
| 1516 |
+
�1 + zr1 − zc
|
| 1517 |
+
0
|
| 1518 |
+
0
|
| 1519 |
+
1 + zr2
|
| 1520 |
+
�
|
| 1521 |
+
.
|
| 1522 |
+
Without loss of generality, we can assume b1 ≤ b2. By (1.4), we have r1 = 2c, r2 = 3c, b1 = 2c−a,
|
| 1523 |
+
and b2 = 3c − a.
|
| 1524 |
+
15
|
| 1525 |
+
|
| 1526 |
+
Lemma 3.8. Suppose that
|
| 1527 |
+
A+(1) =
|
| 1528 |
+
� 2
|
| 1529 |
+
−1
|
| 1530 |
+
−1
|
| 1531 |
+
1
|
| 1532 |
+
�
|
| 1533 |
+
,
|
| 1534 |
+
A−(1) =
|
| 1535 |
+
�2
|
| 1536 |
+
0
|
| 1537 |
+
0
|
| 1538 |
+
2
|
| 1539 |
+
�
|
| 1540 |
+
.
|
| 1541 |
+
Then
|
| 1542 |
+
A+(z) =
|
| 1543 |
+
�
|
| 1544 |
+
1 + z2r
|
| 1545 |
+
−za
|
| 1546 |
+
−z2r−a
|
| 1547 |
+
1 + z2r
|
| 1548 |
+
�
|
| 1549 |
+
,
|
| 1550 |
+
A−(z) =
|
| 1551 |
+
�
|
| 1552 |
+
1 + z2r
|
| 1553 |
+
0
|
| 1554 |
+
0
|
| 1555 |
+
1 + z2r
|
| 1556 |
+
�
|
| 1557 |
+
for some r, a.
|
| 1558 |
+
Proof. We can set
|
| 1559 |
+
A+(z) =
|
| 1560 |
+
�
|
| 1561 |
+
1 + zr1
|
| 1562 |
+
−za
|
| 1563 |
+
−zb
|
| 1564 |
+
1 + zr2
|
| 1565 |
+
�
|
| 1566 |
+
,
|
| 1567 |
+
A−(z) =
|
| 1568 |
+
�1 + zr1
|
| 1569 |
+
0
|
| 1570 |
+
0
|
| 1571 |
+
1 + zr2
|
| 1572 |
+
�
|
| 1573 |
+
.
|
| 1574 |
+
By (1.4), we have r1 = r2 = a + b = 2c.
|
| 1575 |
+
Proof of Theorem 1.5 (2). The remaining possibilities for finite type A±(z) ∈ Y, up to a per-
|
| 1576 |
+
mutation of indices and change of sign, are the six families of the pairs given in Lemma 3.5–3.8,
|
| 1577 |
+
which contain the parameters r, a. We can verify that these six families belong to Y, and they
|
| 1578 |
+
can be reduced to the pairs in Table 1 by change of slices.
|
| 1579 |
+
References
|
| 1580 |
+
[1] George E. Andrews. An analytic generalization of the Rogers-Ramanujan identities for odd moduli. Proc.
|
| 1581 |
+
Nat. Acad. Sci. U.S.A., 71:4082–4085, 1974.
|
| 1582 |
+
[2] Thomas Br¨ustle, Gr´egoire Dupont, and Matthieu P´erotin. On maximal green sequences. Int. Math. Res.
|
| 1583 |
+
Not. IMRN, (16):4547–4586, 2014.
|
| 1584 |
+
[3] Frank Calegari, Stavros Garoufalidis, and Don Zagier. Bloch groups, algebraic K-theory, units, and Nahm’s
|
| 1585 |
+
conjecture. arXiv preprint arXiv:1712.04887, 2017.
|
| 1586 |
+
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|
| 1587 |
+
A(2)
|
| 1588 |
+
2n -modules. J. Pure Appl. Algebra, 220(5):1752–1784, 2016.
|
| 1589 |
+
[5] Peigen Cao, Min Huang, and Fang Li. A conjecture on C-matrices of cluster algebras. Nagoya Math. J.,
|
| 1590 |
+
238:37–46, 2020.
|
| 1591 |
+
[6] Ivan Cherednik and Boris Feigin. Rogers-Ramanujan type identities and Nil-DAHA. Adv. Math., 248:1050–
|
| 1592 |
+
1088, 2013.
|
| 1593 |
+
[7] Sergey Fomin and Andrei Zelevinsky. Cluster algebras. I. Foundations. J. Amer. Math. Soc., 15(2):497–529,
|
| 1594 |
+
2002.
|
| 1595 |
+
[8] Sergey Fomin and Andrei Zelevinsky. Cluster algebras. II. Finite type classification. Invent. Math., 154(1):63–
|
| 1596 |
+
121, 2003.
|
| 1597 |
+
[9] Sergey Fomin and Andrei Zelevinsky. Y -systems and generalized associahedra. Ann. of Math. (2), 158(3):977–
|
| 1598 |
+
1018, 2003.
|
| 1599 |
+
[10] Sergey Fomin and Andrei Zelevinsky. Cluster algebras. IV. Coefficients. Compos. Math., 143(1):112–164,
|
| 1600 |
+
2007.
|
| 1601 |
+
[11] Allan P. Fordy and Robert J. Marsh. Cluster mutation-periodic quivers and associated Laurent sequences.
|
| 1602 |
+
J. Algebraic Combin., 34(1):19–66, 2011.
|
| 1603 |
+
[12] Pavel Galashin and Pavlo Pylyavskyy. The classification of Zamolodchikov periodic quivers. Amer. J. Math.,
|
| 1604 |
+
141(2):447–484, 2019.
|
| 1605 |
+
[13] Stavros Garoufalidis and Don Zagier. Knots, perturbative series and quantum modularity. arXiv preprint
|
| 1606 |
+
arXiv:2111.06645, 2021.
|
| 1607 |
+
[14] Goro Hatayama, Atsuo Kuniba, Masato Okado, Taichiro Takagi, and Zengo Tsuboi. Paths, crystals and
|
| 1608 |
+
fermionic formulae. In MathPhys odyssey, 2001, volume 23 of Prog. Math. Phys., pages 205–272. Birkh¨auser
|
| 1609 |
+
Boston, Boston, MA, 2002.
|
| 1610 |
+
16
|
| 1611 |
+
|
| 1612 |
+
[15] Rei Inoue, Osamu Iyama, Bernhard Keller, Atsuo Kuniba, and Tomoki Nakanishi. Periodicities of T-systems
|
| 1613 |
+
and Y-systems, dilogarithm identities, and cluster algebras I: type Br. Publ. Res. Inst. Math. Sci., 49(1):1–42,
|
| 1614 |
+
2013.
|
| 1615 |
+
[16] Rei Inoue, Osamu Iyama, Bernhard Keller, Atsuo Kuniba, and Tomoki Nakanishi. Periodicities of T-systems
|
| 1616 |
+
and Y-systems, dilogarithm identities, and cluster algebras II: types Cr, F4, and G2. Publ. Res. Inst. Math.
|
| 1617 |
+
Sci., 49(1):43–85, 2013.
|
| 1618 |
+
[17] Victor G. Kac and Dale H. Peterson. Infinite-dimensional Lie algebras, theta functions and modular forms.
|
| 1619 |
+
Adv. in Math., 53(2):125–264, 1984.
|
| 1620 |
+
[18] Akishi Kato and Yuji Terashima.
|
| 1621 |
+
Quiver mutation loops and partition q-series.
|
| 1622 |
+
Comm. Math. Phys.,
|
| 1623 |
+
336(2):811–830, 2015.
|
| 1624 |
+
[19] Bernhard Keller. On cluster theory and quantum dilogarithm identities. In Representations of algebras and
|
| 1625 |
+
related topics, EMS Ser. Congr. Rep., pages 85–116. Eur. Math. Soc., Z¨urich, 2011.
|
| 1626 |
+
[20] Bernhard Keller. Cluster algebras and derived categories. In Derived categories in algebraic geometry, EMS
|
| 1627 |
+
Ser. Congr. Rep., pages 123–183. Eur. Math. Soc., Z¨urich, 2012.
|
| 1628 |
+
[21] Bernhard Keller. The periodicity conjecture for pairs of Dynkin diagrams. Ann. of Math. (2), 177(1):111–170,
|
| 1629 |
+
2013.
|
| 1630 |
+
[22] A. Kuniba and T. Nakanishi. Spectra in conformal field theories from the Rogers dilogarithm. Modern Phys.
|
| 1631 |
+
Lett. A, 7(37):3487–3494, 1992.
|
| 1632 |
+
[23] Chul-hee Lee. Nahm’s conjecture and Y -systems. Commun. Number Theory Phys., 7(1):1–14, 2013.
|
| 1633 |
+
[24] Yuma Mizuno. Difference equations arising from cluster algebras. J. Algebraic Combin., 54(1):295–351, 2021.
|
| 1634 |
+
[25] Kentaro Nagao.
|
| 1635 |
+
Quantum dilogarithm identities.
|
| 1636 |
+
In Infinite analysis 2010—Developments in quantum
|
| 1637 |
+
integrable systems, RIMS Kˆokyˆuroku Bessatsu, B28, pages 165–170. Res. Inst. Math. Sci. (RIMS), Kyoto,
|
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|
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|
| 1668 |
+
17
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| 1669 |
+
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|
| 1 |
+
arXiv:2301.02381v1 [math.NT] 6 Jan 2023
|
| 2 |
+
Existence of primitive pairs with two
|
| 3 |
+
prescribed traces over finite fields
|
| 4 |
+
Aakash Choudhary∗and R. K. Sharma †
|
| 5 |
+
Department of Mathematics,
|
| 6 |
+
Indian Institute of Technology Delhi-110016, India
|
| 7 |
+
Abstract
|
| 8 |
+
Given F = Fpt, a field with pt elements, where p is a prime power,
|
| 9 |
+
t ≥ 7, n are positive integers and f = f1/f2 is a rational func-
|
| 10 |
+
tion, where f1, f2 are relatively prime, irreducible polynomials with
|
| 11 |
+
deg(f1) + deg(f2) = n in F[x]. We construct a sufficient condition on
|
| 12 |
+
(p, t) which guarantees primitive pairing (ǫ, f(ǫ)) exists in F such that
|
| 13 |
+
TrFpt/Fp(ǫ) = a and TrFpt/Fp(f(ǫ)) = b for any prescribed a, b ∈ Fp.
|
| 14 |
+
Further, we demonstrate for any positive integer n, such a pair defi-
|
| 15 |
+
nitely exists for large t. The scenario when n = 2 is handled separately
|
| 16 |
+
and we verified that such a pair exists for all (p, t) except from possible
|
| 17 |
+
71 values of p. A result for the case n = 3 is given as well.
|
| 18 |
+
Keywords: Character, Finite fields, Primitive elements.
|
| 19 |
+
2020 Mathematics Subject Classification: 12E20, 11T23
|
| 20 |
+
1
|
| 21 |
+
Introduction
|
| 22 |
+
Let Fp represent a field of finite order p, where p = qr for some prime q and
|
| 23 |
+
r, a positive integer. The multiplicative group of Fp is cyclic, it is denoted
|
| 24 |
+
by F∗
|
| 25 |
+
p and a generator of F∗
|
| 26 |
+
p is referred to as a primitive element in Fp.
|
| 27 |
+
∗email: achoudhary1396@gmail.com
|
| 28 |
+
†email: rksharmaiitd@gmail.com
|
| 29 |
+
1
|
| 30 |
+
|
| 31 |
+
The field Fp has φ(p − 1) primitive elements, where φ is the Euler’s totient
|
| 32 |
+
function. Let Fpt denote an extension of Fp of degree t for some positive
|
| 33 |
+
integer t. A necessary and sufficient condition for an element ǫ ∈ F∗
|
| 34 |
+
pt to be
|
| 35 |
+
primitive is that it is a root of an irreducible polynomial of degree t over Fp
|
| 36 |
+
and such an irreducible polynomial is referred to as primitive polynomial.
|
| 37 |
+
For ǫ ∈ Fpt, the trace of ǫ over Fp denoted by TrFpt/Fp(ǫ), is defined as
|
| 38 |
+
TrFpt/Fp(ǫ) = ǫ + ǫp + ǫp2 + · · · + ǫpt−1.
|
| 39 |
+
In Cryptographic schemes such as Elgamel encryption scheme and the
|
| 40 |
+
Diffie-Hellman key exchange, primitive elements serve as the fundamental
|
| 41 |
+
building blocks. Numerous applications of primitive elements can be found
|
| 42 |
+
in Coding theory and Cryptography [10], making the study of primitive el-
|
| 43 |
+
ements and primitive polynomials an active research field. Please refer to
|
| 44 |
+
[9] for more information about the existence of primitive elements in finite
|
| 45 |
+
fields. For any rational function f(x) ∈ Fp(x) and ǫ ∈ Fp we call the pair
|
| 46 |
+
(ǫ, f(ǫ)), a primitive pair if both ǫ and f(ǫ) are primitive elements in Fp.
|
| 47 |
+
In general, if ǫ is primitive, f(ǫ) need not be primitive. For instance, take
|
| 48 |
+
x2 + 3x + 2 ∈ F7[x], then 3, 5 are primitive elements in F7 but none of f(3)
|
| 49 |
+
and f(5) are.
|
| 50 |
+
In 1985, Cohen [3] introduced the term ”primitive pair” and he verified
|
| 51 |
+
the existence of primitive pairs (ǫ, f(ǫ)) in Fp for linear polynomials f(x) =
|
| 52 |
+
x + k ∈ Fp[x]. Since then many researchers have conducted studies in this
|
| 53 |
+
area [12, 13, 7, 14].
|
| 54 |
+
Most recently, Cohen, Sharma and Sharma [4] have
|
| 55 |
+
supplied a condition that ensures the occurrence of primitive pair (ǫ, f(ǫ)) in
|
| 56 |
+
Fp for non-exceptional rational function f, i.e., f is not of the form cxjgk(x),
|
| 57 |
+
where j ∈ Z, k > 1 that divides p − 1 and c ∈ F∗
|
| 58 |
+
p, for any g(x) ∈ Fp(x).
|
| 59 |
+
Jungnickel, Vanstone [8] identified a sufficient condition for the occurrence
|
| 60 |
+
of primitive elements ǫ ∈ Fpt with a prescribed trace of ǫ. Later Cohen [5]
|
| 61 |
+
extended the result with some exceptions.
|
| 62 |
+
Chou and Cohen [2], in 2014,
|
| 63 |
+
addressed the issue of the existence of primitive element ǫ ∈ Fpt such that
|
| 64 |
+
TrFpt/Fp(ǫ) = TrFpt/Fp(ǫ−1) = 0. Cao and Wang [1], for t ≥ 29, established
|
| 65 |
+
a condition for the existence of primitive pair (ǫ, f(ǫ)) with f(x) = x2+1
|
| 66 |
+
x
|
| 67 |
+
∈
|
| 68 |
+
Fpt(x) such that for prescribed a, b ∈ F∗
|
| 69 |
+
p, TrFpt/Fp(ǫ) = a and TrFpt/Fp(ǫ−1) =
|
| 70 |
+
b. In 2018, Gupta, Sharma and Cohen [7], for the same rational function
|
| 71 |
+
and prescribed a ∈ Fp, presented a condition that ensures the existence
|
| 72 |
+
of primitive pair (ǫ, f(ǫ)) in Fpt with TrFpt/Fp(ǫ) = a for t ≥ 5. Then in
|
| 73 |
+
2019, Gupta and Sharma [14] extended the result to the rational function
|
| 74 |
+
2
|
| 75 |
+
|
| 76 |
+
ΓM(x) =
|
| 77 |
+
a11x2+a12x+a13
|
| 78 |
+
a22x+a23
|
| 79 |
+
, where M =
|
| 80 |
+
�
|
| 81 |
+
a11
|
| 82 |
+
a12
|
| 83 |
+
a13
|
| 84 |
+
0
|
| 85 |
+
a22
|
| 86 |
+
a23
|
| 87 |
+
�
|
| 88 |
+
∈ M2×3(Fpt) is any
|
| 89 |
+
matrix of rank 2, and if ΓM(x) = λx or λx2 for some λ ∈ Fpt, then λ = 1.
|
| 90 |
+
In 2021, Sharma and Sharma [11] examined the rational function f = f1/f2
|
| 91 |
+
in Fpt(x), where f1 and f2 are relatively prime, irreducible polynomials and
|
| 92 |
+
proved that for prescribed a, b ∈ Fp, the existence of primitive pair (ǫ, f(ǫ))
|
| 93 |
+
in Fpt such that TrFpt/Fp(ǫ) = a and TrFpt/Fp(ǫ−1) = b for t ≥ 7.
|
| 94 |
+
Prior to this article, for primitive pairs, traces were considered for ǫ and
|
| 95 |
+
ǫ−1. In this article, we will consider the trace onto the element ǫ and its
|
| 96 |
+
image under f, i.e, f(ǫ). Some terminology and conventions are introduced
|
| 97 |
+
for explanation. We say that a non-zero polynomial f over Fp[x] has degree
|
| 98 |
+
k ≥ 0, if f(x) = akxk + ak−1xk−1 + · · ·+ a1x + a0, where ak ̸= 0 and we write
|
| 99 |
+
the degree of f as deg(f) = k. Next, we suppose that, for a rational function
|
| 100 |
+
f(x) = f1(x)
|
| 101 |
+
f2(x) ∈ Fp(x), f1 and f2 are relatively prime, irreducible polynomials
|
| 102 |
+
and define the degree-sum as degsum(f) = deg(f1) + deg(f2). We will now
|
| 103 |
+
define various sets that will play a crucial role in this article.
|
| 104 |
+
1. We define Rp,t(n1, n2) to represent the set of all rational function f(x) =
|
| 105 |
+
f1(x)
|
| 106 |
+
f2(x) ∈ Fpt(x) such that f1 and f2 are relatively prime, irreducible
|
| 107 |
+
polynomials over Fpt with deg(f1) = n1 and deg(f2) = n2.
|
| 108 |
+
2. Denote An1,n2 as the set consisting of pairs (p, t) ∈ N × N such that
|
| 109 |
+
for any f ∈ Rp,t(n1, n2) and prescribed a, b ∈ Fp, Fpt contains an ele-
|
| 110 |
+
ment ǫ such that (ǫ, f(ǫ)) is a primitive pair with TrFpt/Fp(ǫ) = a and
|
| 111 |
+
TrFpt/Fp(f(ǫ)) = b.
|
| 112 |
+
3. Define, Rp,t(n) = �
|
| 113 |
+
n1+n2=n Rp,t(n1, n2) and An = �
|
| 114 |
+
n1+n2=n An1,n2.
|
| 115 |
+
First, in this paper, for n ∈ N, we consider f(x) ∈ Rp,t(n) and a, b ∈ Fp,
|
| 116 |
+
and then verify that there exists an element ǫ ∈ Fpt such that (ǫ, f(ǫ)) is
|
| 117 |
+
a primitive pair in Fpt with TrFpt/Fp(ǫ) = a and TrFpt/Fp(f(ǫ)) = b, i.e., we
|
| 118 |
+
provide a sufficient condition on pt such that (p, t) ∈ An. Furthermore, using
|
| 119 |
+
a sieve variation of this sufficient condition, we prove the following result:
|
| 120 |
+
Theorem 1.1. Let t, q, r, p ∈ N be such that q is a prime number, t ≥ 7
|
| 121 |
+
and p = qr. Suppose p and t assumes none of the following values:
|
| 122 |
+
1. 2 ≤ p ≤ 16 or p = 19, 23, 25, 27, 31, 37, 43, 49, 61, 67, 79 and t = 7;
|
| 123 |
+
3
|
| 124 |
+
|
| 125 |
+
2. 2 ≤ p ≤ 31 or p = 32, 37, 41, 43, 47, 83 and t = 8;
|
| 126 |
+
3. 2 ≤ p ≤ 8 or p = 11, 16 and t = 9;
|
| 127 |
+
4. p = 2, 3, 4, 5, 7 and t = 10, 12;
|
| 128 |
+
5. p = 2, 3, 4 and t = 11;
|
| 129 |
+
6. p = 2 and t = 14, 15, 16, 18, 20, 24.
|
| 130 |
+
Then (p, t) ∈ A2.
|
| 131 |
+
Note:- The exceptions in above theorem need not be true exceptions, they
|
| 132 |
+
are possible exceptions.
|
| 133 |
+
SageMath [16] is used to perform all nontrivial calculations required
|
| 134 |
+
throughout this article.
|
| 135 |
+
2
|
| 136 |
+
Preliminaries
|
| 137 |
+
In this section, we present some basic concepts, notations, and results that
|
| 138 |
+
will be used in forthcoming sections of this article. Throughout the article,
|
| 139 |
+
t is a positive integer, p is an arbitrary prime power and Fp is a finite field
|
| 140 |
+
of order p.
|
| 141 |
+
2.1
|
| 142 |
+
Definitions
|
| 143 |
+
1. A character of a finite abelian group G is a homomorphism χ from the
|
| 144 |
+
set G into Z1, where Z1 is the set of all elements of complex field C with
|
| 145 |
+
absolute value 1. The trivial character of G denoted by χ0, is defined
|
| 146 |
+
as χ0(g) = 1 for all g ∈ G. In addition, the set of all characters of G,
|
| 147 |
+
denoted by ˆG, forms a group under multiplication, which is isomorphic
|
| 148 |
+
to G. The order of a character χ is the least positive integer d such
|
| 149 |
+
that χd = χ0. For a finite field Fpt, a character of the additive group
|
| 150 |
+
Fpt is called an additive character and that of the multiplicative group
|
| 151 |
+
F∗
|
| 152 |
+
pt is called a multiplicative character.
|
| 153 |
+
2. For u, a divisor of pt−1, an element ζ ∈ F∗
|
| 154 |
+
pt is called u-free, if whenever
|
| 155 |
+
ζ = ξs, where ξ ∈ Fpt and s|u implies s = 1. We see that an element
|
| 156 |
+
ζ ∈ F∗
|
| 157 |
+
pt is (pt − 1)-free if and only if it is a primitive element of Fpt.
|
| 158 |
+
4
|
| 159 |
+
|
| 160 |
+
For more information on characters, primitive elements and finite fields, we
|
| 161 |
+
refer the reader to [9].
|
| 162 |
+
The following conclusion holds as a particular case of [15, Lemma 10]:
|
| 163 |
+
Lemma 2.1. Let u be a divisor of pt − 1, ζ ∈ F∗
|
| 164 |
+
pt, then we have:
|
| 165 |
+
�
|
| 166 |
+
s|u
|
| 167 |
+
µ(s)
|
| 168 |
+
φ(s)
|
| 169 |
+
�
|
| 170 |
+
χs
|
| 171 |
+
χs(ζ) =
|
| 172 |
+
�
|
| 173 |
+
u
|
| 174 |
+
φ(u)
|
| 175 |
+
if ζ is u − free,
|
| 176 |
+
0
|
| 177 |
+
otherwise
|
| 178 |
+
where µ(.) is the Mobius function and φ(.) is the Euler function, χs runs
|
| 179 |
+
through all the φ(s) multiplicative characters over F∗
|
| 180 |
+
pt with order s.
|
| 181 |
+
Therefore for u, a divisor of pt − 1
|
| 182 |
+
ρu : ǫ �→ θ(u)
|
| 183 |
+
�
|
| 184 |
+
s|u
|
| 185 |
+
µ(s)
|
| 186 |
+
φ(s)
|
| 187 |
+
�
|
| 188 |
+
χs
|
| 189 |
+
χs(ǫ)
|
| 190 |
+
(1)
|
| 191 |
+
gives a characteristic function for the subset of u-free elements of F∗
|
| 192 |
+
pt, where
|
| 193 |
+
θ(u) = φ(u)/u.
|
| 194 |
+
Also for a ∈ Fp,
|
| 195 |
+
τa : ǫ �→ 1
|
| 196 |
+
p
|
| 197 |
+
�
|
| 198 |
+
ψ∈ ˆ
|
| 199 |
+
Fp
|
| 200 |
+
ψ(TrFpt/Fp(ǫ) − a)
|
| 201 |
+
(2)
|
| 202 |
+
is a characteristic function for the subset of Fpt whose elements satisfy
|
| 203 |
+
TrFpt/Fp(ǫ) = a. From [9, Theorem 5.7], any additive character ψ of Fp can
|
| 204 |
+
be derived by ψ(a) = ψ0(ua), where ψ0 is the canonical additive character of
|
| 205 |
+
Fp and u is an element of Fp corresponding to ψ. Thus
|
| 206 |
+
τa = 1
|
| 207 |
+
p
|
| 208 |
+
�
|
| 209 |
+
ψ∈ ˆ
|
| 210 |
+
Fp
|
| 211 |
+
ψ0(TrFpt/Fp(uǫ) − ua)
|
| 212 |
+
= 1
|
| 213 |
+
p
|
| 214 |
+
�
|
| 215 |
+
u∈Fp
|
| 216 |
+
ˆψ0(uǫ)ψ0(−ua)
|
| 217 |
+
(3)
|
| 218 |
+
where ˆψ0 is the additive character of Fpt defined by ˆψ0(ǫ) = ψ0(TrFpt/Fp(ǫ)).
|
| 219 |
+
In next theorem, we will make major use of the results given below by Wang
|
| 220 |
+
and Fu [6] in 2014.
|
| 221 |
+
5
|
| 222 |
+
|
| 223 |
+
Lemma 2.2. [6, Theorem 5.5] Let F(x) ∈ Fpd(x) be a rational function.
|
| 224 |
+
Write F(x) = �k
|
| 225 |
+
j=1 fj(x)rj, where fj(x) ∈ Fpd[x] are irreducible polynomials
|
| 226 |
+
and rj are non zero integers.
|
| 227 |
+
Let χ be a multiplicative character of Fpd.
|
| 228 |
+
Suppose that the rational function �d−1
|
| 229 |
+
i=1 f(xpi) is not of the form h(x)ord(χ) ∈
|
| 230 |
+
Fpd(x), where ord(χ) is the order of χ, Then we have
|
| 231 |
+
����
|
| 232 |
+
�
|
| 233 |
+
ǫ∈Fp,f(ǫ)̸=0,∞
|
| 234 |
+
χ(F(ǫ))
|
| 235 |
+
���� ≤
|
| 236 |
+
�
|
| 237 |
+
d
|
| 238 |
+
k
|
| 239 |
+
�
|
| 240 |
+
j=1
|
| 241 |
+
deg(fj) − 1
|
| 242 |
+
�
|
| 243 |
+
p
|
| 244 |
+
1
|
| 245 |
+
2.
|
| 246 |
+
Lemma 2.3. [6, Theorem 5.6] Let f(x), g(x) ∈ Fpt(x) be rational functions.
|
| 247 |
+
Write f(x) = �k
|
| 248 |
+
j=1 fj(x)rj, where fj(x) ∈ Fpt[x] are irreducible polynomials
|
| 249 |
+
and rj are non-zero integers. Let D1 = �k
|
| 250 |
+
j=1 deg(fj), D2 = max{deg(g), 0},
|
| 251 |
+
D3 is the degree of denominator of g(x) and D4 is the sum of degrees of those
|
| 252 |
+
irreducible polynomials dividing denominator of g but distinct from fj(x)( j=
|
| 253 |
+
1,2,...,k). Let χ be a multiplicative character of Fpt, and let ψ be a nontrivial
|
| 254 |
+
additive character of Fpt. Suppose g(x) is not of the form v(x)pt − v(x) in
|
| 255 |
+
Fpt(x). Then we have
|
| 256 |
+
����
|
| 257 |
+
�
|
| 258 |
+
ǫ∈Fpt,f(ǫ)̸=0,∞,g(ǫ)̸=∞
|
| 259 |
+
χ(f(ǫ))ψ(g(ǫ))
|
| 260 |
+
���� ≤ (D1 + D2 + D3 + D4 − 1)p
|
| 261 |
+
t
|
| 262 |
+
2.
|
| 263 |
+
Evidently, both the sufficient condition (Theorem 3.1) and its sieving
|
| 264 |
+
variation (Theorem 3.4) are entirely dependent on pt and the degrees of the
|
| 265 |
+
numerator and denominator polynomials of the rational function. It is easy
|
| 266 |
+
to see that the Trace part of the main result in [11] is a special case of our
|
| 267 |
+
finding for f(x) = 1
|
| 268 |
+
x.
|
| 269 |
+
For every κ ∈ N, we will use ω(κ) to represent the number of distinct
|
| 270 |
+
prime divisors of κ, and W(κ) to represent the number of square free divisors
|
| 271 |
+
of κ. Clearly, W(κ) = 2ω(κ).
|
| 272 |
+
3
|
| 273 |
+
Sufficient Condition
|
| 274 |
+
Let k1, k2, p, t ∈ N be such that p is a prime power and k1, k2 are positive
|
| 275 |
+
integers which divide pt − 1. Let a, b ∈ Fp, f(x) ∈ Rp,t(n). Let Af,a,b(k1, k2)
|
| 276 |
+
represents the set consisting of all those elements ǫ ∈ Fpt such that ǫ is k1-free,
|
| 277 |
+
f(ǫ) is k2-free, TrFpt/Fp(ǫ) = a, and TrFpt/Ft(f(ǫ)) = b.
|
| 278 |
+
We now verify the sufficient condition as follows:
|
| 279 |
+
6
|
| 280 |
+
|
| 281 |
+
Theorem 3.1. Suppose t, n, p ∈ N and p is a prime power. Suppose that
|
| 282 |
+
p
|
| 283 |
+
t
|
| 284 |
+
2−2 > (2n + 1)W(pt − 1)2.
|
| 285 |
+
Then (p, t) ∈ An.
|
| 286 |
+
Proof. In order to prove this result it suffices to demonstrate that Af,a,b(k1, k2) >
|
| 287 |
+
0 for every f(x) ∈ Rp,t(n) and for every prescribed a, b ∈ Fp . Suppose that
|
| 288 |
+
f(x) ∈ Rp,t(n) be a rational function and that a, b ∈ Fp. Let P represent the
|
| 289 |
+
collection of zeroes and poles of f(x) ∈ Fpt and P
|
| 290 |
+
′ = P ∪ {0}. Let k1, k2 be
|
| 291 |
+
divisors of pt − 1. Then by definition, Af,a,b(k1, k2) will be given by
|
| 292 |
+
Af,a,b(k1, k2) =
|
| 293 |
+
�
|
| 294 |
+
ǫ∈Fpt−P ′
|
| 295 |
+
ρk1(ǫ)ρk2(f(ǫ))τa(ǫ)τb(f(ǫ)).
|
| 296 |
+
Using the characteristic functions (1) and (3) defined in the previous section,
|
| 297 |
+
we obtain
|
| 298 |
+
Af,a,b(k1, k2) = θ(k1)θ(k2)
|
| 299 |
+
p2
|
| 300 |
+
�
|
| 301 |
+
s1|k1,s2|k2
|
| 302 |
+
µ(s1)µ(s2)
|
| 303 |
+
φ(s1)φ(s2)
|
| 304 |
+
�
|
| 305 |
+
s1,s2
|
| 306 |
+
χf,a,b(s1, s2)
|
| 307 |
+
where θ(ki) = φ(ki)
|
| 308 |
+
ki
|
| 309 |
+
; i = 1, 2 and
|
| 310 |
+
χf,a,b(s1, s2) =
|
| 311 |
+
�
|
| 312 |
+
u,v∈Fp
|
| 313 |
+
ψ0(−au − bv)
|
| 314 |
+
�
|
| 315 |
+
ǫ∈Fpt−P ′
|
| 316 |
+
χs1(ǫ)χs2(ǫ0) ˆψ0(uǫ + vǫ0)
|
| 317 |
+
where ǫ0 = f(ǫ). It follows from [9, Example 5.1] that, for any divisors s1, s2
|
| 318 |
+
of pt − 1, there exist integers m1, m2 with 0 < m1, m2 < pt − 1 such that
|
| 319 |
+
χs1(x) = χpt−1(xm1) and χs2(x) = χpt−1(xm2). Thus
|
| 320 |
+
χf,a,b(s1, s2) =
|
| 321 |
+
�
|
| 322 |
+
u,v∈Fp
|
| 323 |
+
ψ0(−au − bv)
|
| 324 |
+
�
|
| 325 |
+
ǫ∈Fpt−P ′
|
| 326 |
+
χpt−1(ǫm1f(ǫ)m2) ˆψ0(uǫ + vǫ0)
|
| 327 |
+
(4)
|
| 328 |
+
=
|
| 329 |
+
�
|
| 330 |
+
u,v∈Fp
|
| 331 |
+
ψ0(−au − bv)
|
| 332 |
+
�
|
| 333 |
+
ǫ∈Fpt−P ′
|
| 334 |
+
χpt−1(F1(ǫ)) ˆψ0(F2(ǫ)),
|
| 335 |
+
(5)
|
| 336 |
+
where F1(x) = xm1f(x)m2 ∈ Fpt(x) and F2(x) = ux + vf(x) ∈ Fpt(x).
|
| 337 |
+
7
|
| 338 |
+
|
| 339 |
+
First we consider the situation when F2(x) = l(x)pt −l(x) for some l(x) ∈
|
| 340 |
+
Fpt(x), where l(x) = l1(x)
|
| 341 |
+
l2(x) with (l1, l2) = 1. We have, ux+vf1(x)
|
| 342 |
+
f2(x) = l1(x)pt
|
| 343 |
+
l2(x)pt −
|
| 344 |
+
l1(x)
|
| 345 |
+
l2(x), that is,
|
| 346 |
+
f2(x)(l1(x)pt − l1(x)l2(x)pt−1) = l2(x)pt(uxf2(x) + vf1(x)).
|
| 347 |
+
Since (l1(x)pt − l1(x)l2(x)pt−1, l2(x)pt) = 1, it implies that, l2(x)pt divides
|
| 348 |
+
f2(x), which can only happen if l2(x) is constant. That is, we have
|
| 349 |
+
c−(pt)f2(x)(l1(x)pt − l1(x)cpt−1) = uxf2(x) + vf1(x)
|
| 350 |
+
where c = l2. Now, the above equation only applies if v = 0. Substituting
|
| 351 |
+
it to the equation above yields, c−(pt)(l1(x)pt − l1(x)cpt−1) = ux, which can
|
| 352 |
+
happen only if l1 is constant and u = 0. Moreover, if F1(x) ̸= r(x)pt−1 for
|
| 353 |
+
any r(x) ∈ Fpt(x), then it follows form Lemma 2.2 that
|
| 354 |
+
|χf,a,b(s1, s2)| ≤ np
|
| 355 |
+
t
|
| 356 |
+
2 +2.
|
| 357 |
+
(6)
|
| 358 |
+
And, when F1(x) = r(x)pt−1 for some r(x) ∈ Fpt(x), where r(x) = r1(x)
|
| 359 |
+
r2(x) is
|
| 360 |
+
such that (r1, r2) = 1. Following [11], it happens only if m1 = m2 = 0, a
|
| 361 |
+
contradiction.
|
| 362 |
+
If F2(x) ̸= d(x)pt − d(x) for any d(x) ∈ Fpt(x) then,
|
| 363 |
+
Case 1 : When n1 ≤ n2. Then in accordance with Lemma 2.3 we have D2
|
| 364 |
+
= 1, and
|
| 365 |
+
|χf,a,b(s1, s2)| ≤ (2n + 1)p
|
| 366 |
+
t
|
| 367 |
+
2 +2.
|
| 368 |
+
(7)
|
| 369 |
+
Case 2 : When n1 > n2. We have D2 = n1 − n2 and
|
| 370 |
+
|χf,a,b(s1, s2)| ≤ 2np
|
| 371 |
+
t
|
| 372 |
+
2+2.
|
| 373 |
+
(8)
|
| 374 |
+
Thus, if (χs1, χs2, u, v) ̸= (χ1, χ1, 0, 0) then based on the discussion above,
|
| 375 |
+
and using (6), (7) and (8), we get, |χf,a,b(s1, s2)| ≤ (2n + 1)p
|
| 376 |
+
t
|
| 377 |
+
2+2. From this
|
| 378 |
+
and the definition of Af,a,b(k1, k2), we get
|
| 379 |
+
Af,a,b(k1, k2) ≥ θ(k1)θ(k2)
|
| 380 |
+
p2
|
| 381 |
+
((pt − |P
|
| 382 |
+
′|) − (2n + 1)p
|
| 383 |
+
t
|
| 384 |
+
2+2(W(k1)W(k2) − 1))
|
| 385 |
+
(9)
|
| 386 |
+
≥ θ(k1)θ(k2)
|
| 387 |
+
p2
|
| 388 |
+
((pt − (n + 1)) − (2n + 1)p
|
| 389 |
+
t
|
| 390 |
+
2+2(W(k1)W(k2) − 1))
|
| 391 |
+
(10)
|
| 392 |
+
8
|
| 393 |
+
|
| 394 |
+
Therefore, if p
|
| 395 |
+
t
|
| 396 |
+
2−2 > (2n + 1)W(k1)W(k2), then Af,a,b(k1, k2) > 0 for every
|
| 397 |
+
f(x) ∈ Rp,t(n) and prescribed a, b ∈ Fp. Considering k1 = k2 = pt − 1, result
|
| 398 |
+
follows.
|
| 399 |
+
Now, we provide the bounds for the absolute values for Af,a,b(mk, k) −
|
| 400 |
+
θ(m)Af,a,b(k, k) and Af,a,b(k, mk) − θ(m)Af,a,b(k, k). Proofs are omitted as
|
| 401 |
+
they follow from the idea of [7].
|
| 402 |
+
Lemma 3.2. Let k be a positive integer that divides pt −1 and m is a prime
|
| 403 |
+
dividing pt − 1 but not k. Then
|
| 404 |
+
|Af,a,b(mk, k) − θ(m)Af,a,b(k, k)| ≤ θ(k)2θ(m)
|
| 405 |
+
p2
|
| 406 |
+
(2n + 1)W(k)2p
|
| 407 |
+
t
|
| 408 |
+
2 +2
|
| 409 |
+
and
|
| 410 |
+
|Af,a,b(k, mk) − θ(m)Af,a,b(k, k)| ≤ θ(k)2θ(m)
|
| 411 |
+
p2
|
| 412 |
+
(2n + 1)W(k)2p
|
| 413 |
+
t
|
| 414 |
+
2+2.
|
| 415 |
+
Lemma 3.3. Let k be a positive integer that divides pt−1 and {q1, q2, . . . , qm}
|
| 416 |
+
be the collection of all primes dividing pt − 1 but not k. Then
|
| 417 |
+
Af,a,b(pt−1, pt−1) ≥
|
| 418 |
+
m
|
| 419 |
+
�
|
| 420 |
+
i=1
|
| 421 |
+
Af,a,b(k, qik)+
|
| 422 |
+
m
|
| 423 |
+
�
|
| 424 |
+
i=1
|
| 425 |
+
Af,a,b(qik, k)−(2m−1)Af,a,b,(k, k).
|
| 426 |
+
Sieve variation of sufficient condition (Theorem 3.1) is given below, proof
|
| 427 |
+
of which is not given as it follows from Lemmas 3.2, 3.3 and ideas in [7].
|
| 428 |
+
Theorem 3.4. Let t, n, p, k ∈ N be such that k divides pt − 1, where p is
|
| 429 |
+
a prime power. Assume {q1, q2, . . . , qm} is the collection of all those primes
|
| 430 |
+
that divide pt −1 but not k. Suppose δ = 1 −2 �m
|
| 431 |
+
i=1
|
| 432 |
+
1
|
| 433 |
+
qi
|
| 434 |
+
and ∆ = 2m − 1
|
| 435 |
+
δ
|
| 436 |
+
+ 2.
|
| 437 |
+
If δ > 0 and
|
| 438 |
+
p
|
| 439 |
+
t
|
| 440 |
+
2 −2 > (2n + 1)∆W(k)2
|
| 441 |
+
then (p, t) ∈ An.
|
| 442 |
+
Lemma 3.5. Suppose that κ ∈ N is such that ω(κ) ≥ 1547, then W(κ) ≤
|
| 443 |
+
κ1/12.
|
| 444 |
+
9
|
| 445 |
+
|
| 446 |
+
Proof. Let V = {2, 3, 5, . . ., 12983} is the set of first 1547 primes. We see
|
| 447 |
+
that the product of all elements of V exceeds K = 6.57 × 105588. Let κ =
|
| 448 |
+
κ1κ2, where κ1 and κ2 are co-prime integers such that all prime divisors
|
| 449 |
+
of κ1 come from the least 1547 prime divisors of κ and remaining prime
|
| 450 |
+
divisors are divisors of κ2. Hence, κ1/12
|
| 451 |
+
1
|
| 452 |
+
> K1/12 > 5.42 × 10465, whereas
|
| 453 |
+
W(κ1) < 4.93 × 10465. The conclusion follows, since ρ1/12 > 2 for all primes
|
| 454 |
+
ρ > 12983.
|
| 455 |
+
We shall need Theorem 3.4 and Lemma 3.5 for calculation work in the
|
| 456 |
+
next section.
|
| 457 |
+
4
|
| 458 |
+
Proof of Theorem 1.1
|
| 459 |
+
Proof will be carried out for the situation t ≥ 7, since according to [2]
|
| 460 |
+
there is no primitive element ǫ, for t ≤ 4, such that TrFpt/Fp(ǫ) = 0 and
|
| 461 |
+
TrFpt/Fp(ǫ−1) = 0. The cases t = 5 and 6 necessitate substantial computation
|
| 462 |
+
and appear to demand a different technique. As a result, we postpone further
|
| 463 |
+
examination of these situations.
|
| 464 |
+
We assume initially that, ω(pt − 1) ≥ 1547.
|
| 465 |
+
Using Theorem 3.1 and
|
| 466 |
+
Lemma 3.5, if p
|
| 467 |
+
t
|
| 468 |
+
2 −2 > 5p
|
| 469 |
+
t
|
| 470 |
+
6, that is, if pt > 5
|
| 471 |
+
3t
|
| 472 |
+
t−6 then (p, t) ∈ A2.
|
| 473 |
+
But
|
| 474 |
+
t ≥ 7 gives
|
| 475 |
+
3t
|
| 476 |
+
t−6 ≤ 21. Hence, if pt > 521 then (p, t) ∈ A2, and this holds
|
| 477 |
+
true for ω(pt − 1) ≥ 1547. Therefore, we may suppose ω(pt − 1) ≤ 1546.
|
| 478 |
+
We shall use sieve variation in order to carry forward computational work.
|
| 479 |
+
Let 62 ≤ ω(pt − 1) ≤ 1546.
|
| 480 |
+
To use Theorem 3.4 assume k to be the
|
| 481 |
+
product of least 62 primes that divide pt − 1, that is, W(k) = 262, then
|
| 482 |
+
m ≤ 1485 and δ assumes its least positive value when {q1, q2, . . . , q1485} =
|
| 483 |
+
{307, 311, 313, . . ., 12979}. This yields δ > 0.004174 and ∆ < 710770.7395.
|
| 484 |
+
Hence 5∆W(k)2 < 7.558211 × 1043. Let Z = 7.558211 × 1043. By sieve
|
| 485 |
+
variation, (p, t) ∈ A2 if q
|
| 486 |
+
t
|
| 487 |
+
2 −2 > Z i.e., if pt > Z
|
| 488 |
+
2t
|
| 489 |
+
t−4. Since t ≥ 7, it gives
|
| 490 |
+
2t
|
| 491 |
+
t−4 ≤ 14
|
| 492 |
+
3 . Therefore, (p, t) ∈ A2 under the condition that pt > 5.834 × 10204.
|
| 493 |
+
Hence, ω(pt − 1) ≥ 95 implies (p, t) ∈ A2. In a similar manner (p, t) ∈ A3,
|
| 494 |
+
A4 if ω(pt − 1) ≥ 95, and (p, t) ∈ A5 if ω(pt − 1) ≥ 96.
|
| 495 |
+
10
|
| 496 |
+
|
| 497 |
+
Table 1.
|
| 498 |
+
Sr.No.
|
| 499 |
+
a ≤ ω(pt − 1) ≤ b
|
| 500 |
+
W(k)
|
| 501 |
+
δ >
|
| 502 |
+
∆ <
|
| 503 |
+
5∆W(k)2 <
|
| 504 |
+
1
|
| 505 |
+
a = 13, b = 94
|
| 506 |
+
213
|
| 507 |
+
0.04481712
|
| 508 |
+
3594.3767988
|
| 509 |
+
1,206,072,718,756
|
| 510 |
+
2
|
| 511 |
+
a = 7, b = 34
|
| 512 |
+
27
|
| 513 |
+
0.04609692
|
| 514 |
+
1151.7513186
|
| 515 |
+
94,351,469
|
| 516 |
+
3
|
| 517 |
+
a = 6, b = 25
|
| 518 |
+
26
|
| 519 |
+
0.08241088
|
| 520 |
+
450.9698124
|
| 521 |
+
9,235,862
|
| 522 |
+
4
|
| 523 |
+
a = 6, b = 23
|
| 524 |
+
26
|
| 525 |
+
0.12550135
|
| 526 |
+
264.9453729
|
| 527 |
+
5,426,082
|
| 528 |
+
5
|
| 529 |
+
a = 6, b = 22
|
| 530 |
+
26
|
| 531 |
+
0.14959773
|
| 532 |
+
209.2223842
|
| 533 |
+
4,284,875
|
| 534 |
+
6
|
| 535 |
+
a = 5, b = 19
|
| 536 |
+
25
|
| 537 |
+
0.07663431
|
| 538 |
+
354.3225878
|
| 539 |
+
1,814,132
|
| 540 |
+
7
|
| 541 |
+
a = 5, b = 17
|
| 542 |
+
25
|
| 543 |
+
0.13927194
|
| 544 |
+
167.1445296
|
| 545 |
+
855,780
|
| 546 |
+
8
|
| 547 |
+
a = 5, b = 16
|
| 548 |
+
25
|
| 549 |
+
0.17317025
|
| 550 |
+
123.2679422
|
| 551 |
+
631,132
|
| 552 |
+
9
|
| 553 |
+
a = 5, b = 15
|
| 554 |
+
25
|
| 555 |
+
0.21090610
|
| 556 |
+
92.0874844
|
| 557 |
+
471,488
|
| 558 |
+
Using the values in the Table 1 above and repeating the process of sieve
|
| 559 |
+
variation, we determine that (p, t) ∈ A2 if pt > (4284875)
|
| 560 |
+
14
|
| 561 |
+
3 or pt > 8.8929 ×
|
| 562 |
+
1030 for t ≥ 7 and since t ≥ 8 implies
|
| 563 |
+
2t
|
| 564 |
+
t−4 ≤ 4, so (p, t) ∈ A2 if pt > 3.371×1026
|
| 565 |
+
for t ≥ 8.
|
| 566 |
+
Therefore, for t ≥ 8 it is sufficient that ω(pt − 1) ≥ 20, We deduce,
|
| 567 |
+
utilising sieve variation repeatedly for values in the second section of the
|
| 568 |
+
preceding table that, (p, t) ∈ A2 if pt > 1.084 × 1025.
|
| 569 |
+
Similarly, ω(pt − 1) ≥ 18 is sufficient for inclusion of (p, t) in A2, and based
|
| 570 |
+
on the table above (p, t) ∈ A2 if pt > 2.2725 × 1021 for t ≥ 9, and (p, t) ∈ A2
|
| 571 |
+
if pt > 8.158 × 1018 for t ≥ 10.
|
| 572 |
+
Hence (p, t) ∈ A2 unless t = 7 and p < 26382, t = 8 and p < 1347, t = 9
|
| 573 |
+
and p < 237, t = 10 and p < 78, t = 11 and p < 53, t = 12 and p < 38,
|
| 574 |
+
t = 13 and p < 29, t = 14 and p < 23, t = 15 and p < 19, t = 16 and p < 16,
|
| 575 |
+
t = 17 and p < 13, t = 18 and p < 12, t = 19 and p < 10, t = 20 and p < 9,
|
| 576 |
+
t = 21, 22 and p < 8, t = 23, 24 and p < 7, t = 25, 26, 27 and p = 2, 3, 4, 5.
|
| 577 |
+
28 ≤ t ≤ 31 and p = 2, 3, 4. 32 ≤ t ≤ 39 and for p = 2, 3. 40 ≤ t ≤ 62 and
|
| 578 |
+
p = 2.
|
| 579 |
+
From the preceding discussion for every (p, t), we validated Theorem 3.1
|
| 580 |
+
and compiled a list of 570 potential exceptions (listed in the Appendix).
|
| 581 |
+
11
|
| 582 |
+
|
| 583 |
+
Then, for these potential exceptions, we discover that sieve variation is true
|
| 584 |
+
for the large majority of prime powers, with the exception of those mentioned
|
| 585 |
+
in Theorem 1.1.
|
| 586 |
+
(see Appendix).
|
| 587 |
+
Theorem 1.1 derives from this.
|
| 588 |
+
Using
|
| 589 |
+
similar reasoning, it is possible to find a subset of An for any n ∈ N. In
|
| 590 |
+
particular, for A3, we have the following result.
|
| 591 |
+
Theorem 4.1. Suppose t q, r, p ∈ N be such that q is a prime number, t
|
| 592 |
+
≥ 7 and p = qr. Let p and t assumes none of the following values:
|
| 593 |
+
1. 2 ≤ p ≤ 31 or p = 37, 41, 43, 49, 61, 67, 71, 79, 103, 121 and t = 7;
|
| 594 |
+
2. 2 ≤ p ≤ 47 or p = 53, 83 and t = 8;
|
| 595 |
+
3. 2 ≤ p ≤ 7 or p = 9, 11, 16 and t = 9;
|
| 596 |
+
4. 2 ≤ p ≤ 8 and t = 10;
|
| 597 |
+
5. p = 2, 3, 4 and t = 11;
|
| 598 |
+
6. 2 ≤ p ≤ 7 and t = 12;
|
| 599 |
+
7. p = 2 and t = 14, 15, 16, 18, 20, 24.
|
| 600 |
+
Then (p, t) ∈ A3.
|
| 601 |
+
References
|
| 602 |
+
[1] Cao, X., Wang, P. (2014). Primitive elements with prescribed trace.
|
| 603 |
+
AAECC 25(5):339–345.
|
| 604 |
+
[2] Chou, W. S., Cohen, S. D. (2001). Primitive elements with zero traces.
|
| 605 |
+
Finite Fields Appl. 7(1):125–141.
|
| 606 |
+
[3] Cohen, S. D. (1985). Consecutive primitive roots in a finite field. Proc.
|
| 607 |
+
Amer. Math. Soc. 93(2):189–197.
|
| 608 |
+
[4] Cohen, S .D., Sharma, H., Sharma, R. K. (2021). Primitive values of ra-
|
| 609 |
+
tional functions at primitive elements of a finite field. J. Number Theory
|
| 610 |
+
219:237–246.
|
| 611 |
+
[5] Cohen, S. D., Presern, M. (2005). Primitive finite field elements with
|
| 612 |
+
prescribed trace. Southeast Asian Bull. Math. 29(2):283–300.
|
| 613 |
+
12
|
| 614 |
+
|
| 615 |
+
[6] Fu, L., Wan, D. (2014). A class of incomplete character sums. Q. J.
|
| 616 |
+
Math. 65(4):1195–1211.
|
| 617 |
+
[7] Gupta, A., Sharma, R. K., Cohen, S. D. (2018). Primitive element pairs
|
| 618 |
+
with one prescribed trace over a finite field. Finite Fields Appl. 54:1–14.
|
| 619 |
+
[8] Jungnickel, D., Vanstone, S. A. (1989). On primitive polynomials over
|
| 620 |
+
finite fields. J. Algebra 124(2):337–353.
|
| 621 |
+
[9] Lidl, R., Niederreiter, H. (1997). Finite Field, Vol. 20. Cambridge (UK):
|
| 622 |
+
Cambridge University Press.
|
| 623 |
+
[10] Paar, C., Pelzl, J. (2010). Public-Key Cryptosystems Based on the Dis-
|
| 624 |
+
crete Logarithm Problem, pp. 205–238. Berlin, Heidelberg: Springer.
|
| 625 |
+
[11] Sharma, H., Sharma, R.K. (2021). Existence of primitive pairs with
|
| 626 |
+
prescribed traces over finite fields. Commun. Algebra 49(4):1773-1780.
|
| 627 |
+
[12] Sharma, R.K., Awasthi, A., Gupta, A. (2018). Existence of pair of prim-
|
| 628 |
+
itive elements over finite fields of characteristic 2. J. Number Theory
|
| 629 |
+
193:386–394.
|
| 630 |
+
[13] Sharma, R. K., Gupta, A. (2017). Existence of some special primitive
|
| 631 |
+
normal elements over finite fields. Finite Fields Appl. 46:280–303.
|
| 632 |
+
[14] Sharma, R. K., Gupta, A. (2019). Pair of primitive elements with pre-
|
| 633 |
+
scribed traces over finite fields. Commun. Algebra 47(3):1278–1286.
|
| 634 |
+
[15] Shuqin, F., Wenbao, H. (2004). Character sums over galois rings and
|
| 635 |
+
primitive polynomials over finite fields. Finite Fields Appl. 10(1):36–52.
|
| 636 |
+
[16] The Sage Developers, SageMath, the Sage mathematics software system
|
| 637 |
+
(version 9.0), https:// www.sagemath.org, 2020.
|
| 638 |
+
13
|
| 639 |
+
|
| 640 |
+
Appendix
|
| 641 |
+
List of 570 values of (p, t) for which the condition of
|
| 642 |
+
Theorem 3.1 of the this article fails:
|
| 643 |
+
For t=7:
|
| 644 |
+
p= 2, 4, 8, 16, 32, 64, 256, 512, 1024, 4096, 3, 9, 27, 81, 243, 729, 6561, 5,
|
| 645 |
+
25, 125, 625, 3125, 15625, 7, 49, 343, 2401, 11, 121, 1331, 14641, 13, 169,
|
| 646 |
+
2197, 17, 19, 361, 23, 529, 29, 31, 37, 41, 1681, 43, 1849, 47, 53, 59, 3481, 61,
|
| 647 |
+
67, 4489, 71, 79, 6241, 83, 6889, 97, 9409, 101, 103, 10609, 107, 109, 11881,
|
| 648 |
+
113, 127, 131, 17161, 139, 19321, 151, 22801, 157, 181, 191, 197, 199, 211,
|
| 649 |
+
223, 227, 229, 233, 239, 241, 263, 269, 271, 277, 281, 283, 293, 311, 331, 359,
|
| 650 |
+
367, 389, 397, 401, 409, 431, 439, 463, 491, 499, 509, 547, 571, 593, 601, 607,
|
| 651 |
+
613, 619, 631, 643, 659, 661, 683, 691, 709, 727, 733, 739, 743, 877, 919, 953,
|
| 652 |
+
967, 1021, 1051, 1063, 1093, 1123, 1151, 1171, 1181, 1231, 1283, 1301, 1303,
|
| 653 |
+
1321, 1381, 1399, 1453, 1481, 1483, 1499, 1523, 1531, 1597, 1607, 1693, 1723,
|
| 654 |
+
1741, 1759, 1789, 1801, 1823, 1877, 1879, 1951, 2003, 2141, 2161, 2281, 2311,
|
| 655 |
+
2381, 2591, 2713, 2731, 2791, 2887, 2971, 3041, 3083, 3191, 3221, 3229, 3271,
|
| 656 |
+
3301, 3307, 3313, 3499, 3547, 3571, 3739, 3851, 3911, 4013, 4159, 4219, 4241,
|
| 657 |
+
4243, 4261, 4327, 4421, 4423, 4567, 4621, 4663, 4691, 4751, 4957, 5419, 5923,
|
| 658 |
+
5981, 6067, 6211, 6491, 6577, 7159, 7759, 8009, 8053, 8191, 8807, 9103, 9403,
|
| 659 |
+
9421, 9463, 9719, 9767, 9871, 9901, 9967, 10427, 10949, 10957, 10979, 11311,
|
| 660 |
+
11593, 11621, 12959, 14323, 15313, 15511, 16381, 17431, 17491, 19483, 19687,
|
| 661 |
+
19891, 20011, 20441, 21391, 22543, 23143, 23671, 24181, 24683, 25171, 25411.
|
| 662 |
+
For t=8:
|
| 663 |
+
p = 2, 4, 8, 16, 32, 64, 128, 256, 512, 1024, 3, 9, 27, 81, 243, 729, 5, 25, 125,
|
| 664 |
+
7, 49, 343, 11, 121, 1331, 13, 169, 17, 19, 361, 23, 529, 29, 841, 31, 961, 37,
|
| 665 |
+
41, 43, 47, 53, 59, 61, 67, 71, 73, 79, 83, 89, 97, 101, 103, 107, 109, 113, 127,
|
| 666 |
+
131, 137, 139, 149, 151, 157, 163, 167, 173, 179, 181, 191, 193, 197, 211, 223,
|
| 667 |
+
227, 229, 233, 239, 241, 251, 257, 263, 269, 271, 277, 281, 283, 293, 307, 311,
|
| 668 |
+
313, 317, 331, 337, 347, 349, 353, 359, 367, 373, 379, 383, 389, 397, 401, 409,
|
| 669 |
+
419, 421, 433, 439, 443, 457, 461, 463, 467, 491, 499, 509, 521, 523, 541, 547,
|
| 670 |
+
557, 563, 569, 571, 587, 593, 599, 601, 617, 619, 631, 647, 653, 659, 661, 683,
|
| 671 |
+
691, 701, 709, 727, 733, 739, 743, 757, 773, 787, 797, 809, 811, 823, 827, 829,
|
| 672 |
+
839, 853, 857, 859, 863, 881, 887, 911, 919, 929, 937, 941, 947, 953, 967, 971,
|
| 673 |
+
977, 983, 991, 1009, 1013, 1021, 1033, 1039, 1061, 1063, 1069, 1087, 1091,
|
| 674 |
+
14
|
| 675 |
+
|
| 676 |
+
1093, 1097, 1103, 1109, 1117, 1123, 1201, 1213, 1217, 1223, 1231, 1277, 1279,
|
| 677 |
+
1283, 1289, 1291, 1301, 1303, 1319, 1321.
|
| 678 |
+
For t=9:
|
| 679 |
+
p = 2, 4, 8, 16, 32, 3, 9, 27, 81, 5, 25, 125, 7, 49, 11, 121, 13, 169, 17, 19, 23,
|
| 680 |
+
29, 31, 37, 43, 47, 53, 61, 79, 83, 137, 139, 149, 157, 211.
|
| 681 |
+
For t=10:
|
| 682 |
+
p = 2, 4, 8, 16, 32, 64, 3, 9, 27, 5, 25, 7, 49, 11, 13, 17, 19, 23, 29, 31, 37, 41,
|
| 683 |
+
53, 59, 61, 67.
|
| 684 |
+
For t=11:
|
| 685 |
+
p = 2, 4, 16, 3, 9, 7, 13.
|
| 686 |
+
For t=12:
|
| 687 |
+
p = 2, 4, 8, 16, 32, 3, 9, 27, 5, 7, 11, 13, 17, 19, 23, 29, 31, 37.
|
| 688 |
+
For t=14:
|
| 689 |
+
p = 2, 4, 3, 5, 7.
|
| 690 |
+
For t=15:
|
| 691 |
+
p = 2, 4, 16, 3, 9, 5.
|
| 692 |
+
For t=16:
|
| 693 |
+
p = 2, 4, 8, 3, 5.
|
| 694 |
+
For t=18:
|
| 695 |
+
p = 2, 3, 4, 5.
|
| 696 |
+
For t=20:
|
| 697 |
+
p = 2, 4, 8.
|
| 698 |
+
15
|
| 699 |
+
|
| 700 |
+
For t=24:
|
| 701 |
+
p = 2, 3, 4.
|
| 702 |
+
For t=22, 28, 30, 36:
|
| 703 |
+
p = 2.
|
| 704 |
+
16
|
| 705 |
+
|
| 706 |
+
List consisting values of k, m corresponding to (p, t) for
|
| 707 |
+
which the condition of theorem 3.1 fails but sieve vari-
|
| 708 |
+
ation is satisfied for some choice of k in this article.
|
| 709 |
+
for t=7:
|
| 710 |
+
Sr.No.
|
| 711 |
+
p
|
| 712 |
+
k
|
| 713 |
+
m
|
| 714 |
+
1
|
| 715 |
+
32
|
| 716 |
+
1
|
| 717 |
+
4
|
| 718 |
+
2
|
| 719 |
+
64
|
| 720 |
+
3
|
| 721 |
+
5
|
| 722 |
+
3
|
| 723 |
+
256
|
| 724 |
+
3
|
| 725 |
+
7
|
| 726 |
+
4
|
| 727 |
+
512
|
| 728 |
+
1
|
| 729 |
+
6
|
| 730 |
+
5
|
| 731 |
+
1024
|
| 732 |
+
3
|
| 733 |
+
8
|
| 734 |
+
6
|
| 735 |
+
4096
|
| 736 |
+
3
|
| 737 |
+
11
|
| 738 |
+
7
|
| 739 |
+
81
|
| 740 |
+
2
|
| 741 |
+
5
|
| 742 |
+
8
|
| 743 |
+
243
|
| 744 |
+
2
|
| 745 |
+
4
|
| 746 |
+
9
|
| 747 |
+
729
|
| 748 |
+
2
|
| 749 |
+
7
|
| 750 |
+
10
|
| 751 |
+
6561
|
| 752 |
+
2
|
| 753 |
+
8
|
| 754 |
+
11
|
| 755 |
+
125
|
| 756 |
+
2
|
| 757 |
+
4
|
| 758 |
+
12
|
| 759 |
+
625
|
| 760 |
+
6
|
| 761 |
+
5
|
| 762 |
+
13
|
| 763 |
+
3125
|
| 764 |
+
2
|
| 765 |
+
7
|
| 766 |
+
14
|
| 767 |
+
15625
|
| 768 |
+
6
|
| 769 |
+
10
|
| 770 |
+
15
|
| 771 |
+
343
|
| 772 |
+
6
|
| 773 |
+
4
|
| 774 |
+
16
|
| 775 |
+
2401
|
| 776 |
+
6
|
| 777 |
+
6
|
| 778 |
+
17
|
| 779 |
+
121
|
| 780 |
+
6
|
| 781 |
+
4
|
| 782 |
+
18
|
| 783 |
+
1331
|
| 784 |
+
2
|
| 785 |
+
8
|
| 786 |
+
19
|
| 787 |
+
14641
|
| 788 |
+
6
|
| 789 |
+
8
|
| 790 |
+
20
|
| 791 |
+
169
|
| 792 |
+
6
|
| 793 |
+
4
|
| 794 |
+
21
|
| 795 |
+
2197
|
| 796 |
+
6
|
| 797 |
+
6
|
| 798 |
+
22
|
| 799 |
+
17
|
| 800 |
+
2
|
| 801 |
+
1
|
| 802 |
+
23
|
| 803 |
+
361
|
| 804 |
+
6
|
| 805 |
+
5
|
| 806 |
+
24
|
| 807 |
+
529
|
| 808 |
+
6
|
| 809 |
+
6
|
| 810 |
+
25
|
| 811 |
+
29
|
| 812 |
+
2
|
| 813 |
+
2
|
| 814 |
+
26
|
| 815 |
+
41
|
| 816 |
+
2
|
| 817 |
+
3
|
| 818 |
+
27
|
| 819 |
+
1681
|
| 820 |
+
6
|
| 821 |
+
6
|
| 822 |
+
28
|
| 823 |
+
1849
|
| 824 |
+
6
|
| 825 |
+
5
|
| 826 |
+
29
|
| 827 |
+
47
|
| 828 |
+
2
|
| 829 |
+
3
|
| 830 |
+
30
|
| 831 |
+
53
|
| 832 |
+
2
|
| 833 |
+
3
|
| 834 |
+
31
|
| 835 |
+
59
|
| 836 |
+
2
|
| 837 |
+
5
|
| 838 |
+
32
|
| 839 |
+
3481
|
| 840 |
+
6
|
| 841 |
+
8
|
| 842 |
+
33
|
| 843 |
+
4489
|
| 844 |
+
6
|
| 845 |
+
8
|
| 846 |
+
Sr.No.
|
| 847 |
+
p
|
| 848 |
+
k
|
| 849 |
+
m
|
| 850 |
+
34
|
| 851 |
+
71
|
| 852 |
+
2
|
| 853 |
+
4
|
| 854 |
+
35
|
| 855 |
+
6241
|
| 856 |
+
6
|
| 857 |
+
8
|
| 858 |
+
36
|
| 859 |
+
83
|
| 860 |
+
2
|
| 861 |
+
3
|
| 862 |
+
37
|
| 863 |
+
6889
|
| 864 |
+
6
|
| 865 |
+
7
|
| 866 |
+
38
|
| 867 |
+
97
|
| 868 |
+
6
|
| 869 |
+
3
|
| 870 |
+
39
|
| 871 |
+
9409
|
| 872 |
+
6
|
| 873 |
+
7
|
| 874 |
+
40
|
| 875 |
+
101
|
| 876 |
+
2
|
| 877 |
+
3
|
| 878 |
+
41
|
| 879 |
+
103
|
| 880 |
+
6
|
| 881 |
+
4
|
| 882 |
+
42
|
| 883 |
+
10609
|
| 884 |
+
6
|
| 885 |
+
7
|
| 886 |
+
43
|
| 887 |
+
107
|
| 888 |
+
2
|
| 889 |
+
4
|
| 890 |
+
44
|
| 891 |
+
109
|
| 892 |
+
6
|
| 893 |
+
3
|
| 894 |
+
45
|
| 895 |
+
11881
|
| 896 |
+
6
|
| 897 |
+
7
|
| 898 |
+
46
|
| 899 |
+
113
|
| 900 |
+
2
|
| 901 |
+
3
|
| 902 |
+
47
|
| 903 |
+
127
|
| 904 |
+
6
|
| 905 |
+
4
|
| 906 |
+
48
|
| 907 |
+
131
|
| 908 |
+
2
|
| 909 |
+
5
|
| 910 |
+
49
|
| 911 |
+
17161
|
| 912 |
+
6
|
| 913 |
+
9
|
| 914 |
+
50
|
| 915 |
+
139
|
| 916 |
+
6
|
| 917 |
+
4
|
| 918 |
+
51
|
| 919 |
+
19321
|
| 920 |
+
6
|
| 921 |
+
9
|
| 922 |
+
52
|
| 923 |
+
151
|
| 924 |
+
6
|
| 925 |
+
3
|
| 926 |
+
53
|
| 927 |
+
22801
|
| 928 |
+
6
|
| 929 |
+
9
|
| 930 |
+
54
|
| 931 |
+
157
|
| 932 |
+
6
|
| 933 |
+
3
|
| 934 |
+
55
|
| 935 |
+
181
|
| 936 |
+
6
|
| 937 |
+
4
|
| 938 |
+
56
|
| 939 |
+
191
|
| 940 |
+
2
|
| 941 |
+
6
|
| 942 |
+
57
|
| 943 |
+
197
|
| 944 |
+
2
|
| 945 |
+
4
|
| 946 |
+
58
|
| 947 |
+
199
|
| 948 |
+
6
|
| 949 |
+
5
|
| 950 |
+
59
|
| 951 |
+
211
|
| 952 |
+
6
|
| 953 |
+
4
|
| 954 |
+
60
|
| 955 |
+
223
|
| 956 |
+
6
|
| 957 |
+
5
|
| 958 |
+
61
|
| 959 |
+
227
|
| 960 |
+
2
|
| 961 |
+
4
|
| 962 |
+
62
|
| 963 |
+
229
|
| 964 |
+
6
|
| 965 |
+
3
|
| 966 |
+
63
|
| 967 |
+
233
|
| 968 |
+
2
|
| 969 |
+
4
|
| 970 |
+
64
|
| 971 |
+
239
|
| 972 |
+
2
|
| 973 |
+
5
|
| 974 |
+
65
|
| 975 |
+
241
|
| 976 |
+
6
|
| 977 |
+
3
|
| 978 |
+
66
|
| 979 |
+
263
|
| 980 |
+
2
|
| 981 |
+
4
|
| 982 |
+
17
|
| 983 |
+
|
| 984 |
+
Sr.No.
|
| 985 |
+
q
|
| 986 |
+
l
|
| 987 |
+
s
|
| 988 |
+
67
|
| 989 |
+
269
|
| 990 |
+
2
|
| 991 |
+
6
|
| 992 |
+
68
|
| 993 |
+
271
|
| 994 |
+
6
|
| 995 |
+
3
|
| 996 |
+
69
|
| 997 |
+
277
|
| 998 |
+
6
|
| 999 |
+
4
|
| 1000 |
+
70
|
| 1001 |
+
281
|
| 1002 |
+
2
|
| 1003 |
+
5
|
| 1004 |
+
71
|
| 1005 |
+
283
|
| 1006 |
+
6
|
| 1007 |
+
3
|
| 1008 |
+
72
|
| 1009 |
+
293
|
| 1010 |
+
2
|
| 1011 |
+
4
|
| 1012 |
+
73
|
| 1013 |
+
311
|
| 1014 |
+
2
|
| 1015 |
+
5
|
| 1016 |
+
74
|
| 1017 |
+
331
|
| 1018 |
+
6
|
| 1019 |
+
4
|
| 1020 |
+
75
|
| 1021 |
+
359
|
| 1022 |
+
2
|
| 1023 |
+
6
|
| 1024 |
+
76
|
| 1025 |
+
367
|
| 1026 |
+
6
|
| 1027 |
+
4
|
| 1028 |
+
77
|
| 1029 |
+
389
|
| 1030 |
+
2
|
| 1031 |
+
6
|
| 1032 |
+
78
|
| 1033 |
+
397
|
| 1034 |
+
6
|
| 1035 |
+
5
|
| 1036 |
+
79
|
| 1037 |
+
401
|
| 1038 |
+
2
|
| 1039 |
+
5
|
| 1040 |
+
80
|
| 1041 |
+
409
|
| 1042 |
+
6
|
| 1043 |
+
4
|
| 1044 |
+
81
|
| 1045 |
+
431
|
| 1046 |
+
2
|
| 1047 |
+
7
|
| 1048 |
+
82
|
| 1049 |
+
439
|
| 1050 |
+
6
|
| 1051 |
+
4
|
| 1052 |
+
83
|
| 1053 |
+
463
|
| 1054 |
+
6
|
| 1055 |
+
4
|
| 1056 |
+
84
|
| 1057 |
+
491
|
| 1058 |
+
2
|
| 1059 |
+
5
|
| 1060 |
+
85
|
| 1061 |
+
499
|
| 1062 |
+
6
|
| 1063 |
+
4
|
| 1064 |
+
86
|
| 1065 |
+
509
|
| 1066 |
+
2
|
| 1067 |
+
5
|
| 1068 |
+
87
|
| 1069 |
+
547
|
| 1070 |
+
6
|
| 1071 |
+
4
|
| 1072 |
+
88
|
| 1073 |
+
571
|
| 1074 |
+
6
|
| 1075 |
+
4
|
| 1076 |
+
89
|
| 1077 |
+
593
|
| 1078 |
+
2
|
| 1079 |
+
5
|
| 1080 |
+
90
|
| 1081 |
+
601
|
| 1082 |
+
6
|
| 1083 |
+
4
|
| 1084 |
+
91
|
| 1085 |
+
607
|
| 1086 |
+
6
|
| 1087 |
+
4
|
| 1088 |
+
92
|
| 1089 |
+
613
|
| 1090 |
+
6
|
| 1091 |
+
5
|
| 1092 |
+
93
|
| 1093 |
+
619
|
| 1094 |
+
6
|
| 1095 |
+
4
|
| 1096 |
+
94
|
| 1097 |
+
631
|
| 1098 |
+
6
|
| 1099 |
+
4
|
| 1100 |
+
95
|
| 1101 |
+
643
|
| 1102 |
+
6
|
| 1103 |
+
4
|
| 1104 |
+
96
|
| 1105 |
+
659
|
| 1106 |
+
2
|
| 1107 |
+
5
|
| 1108 |
+
97
|
| 1109 |
+
661
|
| 1110 |
+
6
|
| 1111 |
+
5
|
| 1112 |
+
98
|
| 1113 |
+
683
|
| 1114 |
+
2
|
| 1115 |
+
5
|
| 1116 |
+
99
|
| 1117 |
+
691
|
| 1118 |
+
6
|
| 1119 |
+
6
|
| 1120 |
+
100
|
| 1121 |
+
709
|
| 1122 |
+
6
|
| 1123 |
+
4
|
| 1124 |
+
101
|
| 1125 |
+
727
|
| 1126 |
+
6
|
| 1127 |
+
5
|
| 1128 |
+
102
|
| 1129 |
+
733
|
| 1130 |
+
6
|
| 1131 |
+
4
|
| 1132 |
+
103
|
| 1133 |
+
739
|
| 1134 |
+
6
|
| 1135 |
+
4
|
| 1136 |
+
104
|
| 1137 |
+
743
|
| 1138 |
+
2
|
| 1139 |
+
5
|
| 1140 |
+
105
|
| 1141 |
+
877
|
| 1142 |
+
6
|
| 1143 |
+
5
|
| 1144 |
+
106
|
| 1145 |
+
919
|
| 1146 |
+
6
|
| 1147 |
+
6
|
| 1148 |
+
Sr.No.
|
| 1149 |
+
q
|
| 1150 |
+
l
|
| 1151 |
+
s
|
| 1152 |
+
107
|
| 1153 |
+
953
|
| 1154 |
+
2
|
| 1155 |
+
8
|
| 1156 |
+
108
|
| 1157 |
+
967
|
| 1158 |
+
6
|
| 1159 |
+
5
|
| 1160 |
+
109
|
| 1161 |
+
1021
|
| 1162 |
+
6
|
| 1163 |
+
5
|
| 1164 |
+
110
|
| 1165 |
+
1051
|
| 1166 |
+
6
|
| 1167 |
+
5
|
| 1168 |
+
111
|
| 1169 |
+
1063
|
| 1170 |
+
6
|
| 1171 |
+
5
|
| 1172 |
+
112
|
| 1173 |
+
1093
|
| 1174 |
+
6
|
| 1175 |
+
5
|
| 1176 |
+
113
|
| 1177 |
+
1123
|
| 1178 |
+
6
|
| 1179 |
+
6
|
| 1180 |
+
114
|
| 1181 |
+
1151
|
| 1182 |
+
2
|
| 1183 |
+
6
|
| 1184 |
+
115
|
| 1185 |
+
1171
|
| 1186 |
+
6
|
| 1187 |
+
5
|
| 1188 |
+
116
|
| 1189 |
+
1181
|
| 1190 |
+
2
|
| 1191 |
+
6
|
| 1192 |
+
117
|
| 1193 |
+
1231
|
| 1194 |
+
6
|
| 1195 |
+
6
|
| 1196 |
+
118
|
| 1197 |
+
1283
|
| 1198 |
+
2
|
| 1199 |
+
6
|
| 1200 |
+
119
|
| 1201 |
+
1301
|
| 1202 |
+
2
|
| 1203 |
+
6
|
| 1204 |
+
120
|
| 1205 |
+
1303
|
| 1206 |
+
6
|
| 1207 |
+
5
|
| 1208 |
+
121
|
| 1209 |
+
1321
|
| 1210 |
+
6
|
| 1211 |
+
5
|
| 1212 |
+
122
|
| 1213 |
+
1381
|
| 1214 |
+
6
|
| 1215 |
+
5
|
| 1216 |
+
123
|
| 1217 |
+
1399
|
| 1218 |
+
6
|
| 1219 |
+
5
|
| 1220 |
+
124
|
| 1221 |
+
1453
|
| 1222 |
+
6
|
| 1223 |
+
5
|
| 1224 |
+
125
|
| 1225 |
+
1481
|
| 1226 |
+
2
|
| 1227 |
+
6
|
| 1228 |
+
126
|
| 1229 |
+
1483
|
| 1230 |
+
6
|
| 1231 |
+
6
|
| 1232 |
+
127
|
| 1233 |
+
1499
|
| 1234 |
+
2
|
| 1235 |
+
6
|
| 1236 |
+
128
|
| 1237 |
+
1523
|
| 1238 |
+
2
|
| 1239 |
+
6
|
| 1240 |
+
129
|
| 1241 |
+
1531
|
| 1242 |
+
6
|
| 1243 |
+
6
|
| 1244 |
+
130
|
| 1245 |
+
1597
|
| 1246 |
+
6
|
| 1247 |
+
5
|
| 1248 |
+
131
|
| 1249 |
+
1607
|
| 1250 |
+
2
|
| 1251 |
+
6
|
| 1252 |
+
132
|
| 1253 |
+
1693
|
| 1254 |
+
6
|
| 1255 |
+
6
|
| 1256 |
+
133
|
| 1257 |
+
1723
|
| 1258 |
+
6
|
| 1259 |
+
5
|
| 1260 |
+
134
|
| 1261 |
+
1741
|
| 1262 |
+
6
|
| 1263 |
+
6
|
| 1264 |
+
135
|
| 1265 |
+
1759
|
| 1266 |
+
6
|
| 1267 |
+
5
|
| 1268 |
+
136
|
| 1269 |
+
1789
|
| 1270 |
+
6
|
| 1271 |
+
5
|
| 1272 |
+
137
|
| 1273 |
+
1801
|
| 1274 |
+
6
|
| 1275 |
+
6
|
| 1276 |
+
138
|
| 1277 |
+
1823
|
| 1278 |
+
2
|
| 1279 |
+
6
|
| 1280 |
+
139
|
| 1281 |
+
1877
|
| 1282 |
+
2
|
| 1283 |
+
6
|
| 1284 |
+
140
|
| 1285 |
+
1879
|
| 1286 |
+
6
|
| 1287 |
+
5
|
| 1288 |
+
141
|
| 1289 |
+
1951
|
| 1290 |
+
6
|
| 1291 |
+
7
|
| 1292 |
+
142
|
| 1293 |
+
2003
|
| 1294 |
+
2
|
| 1295 |
+
7
|
| 1296 |
+
143
|
| 1297 |
+
2141
|
| 1298 |
+
2
|
| 1299 |
+
7
|
| 1300 |
+
144
|
| 1301 |
+
2161
|
| 1302 |
+
6
|
| 1303 |
+
7
|
| 1304 |
+
145
|
| 1305 |
+
2281
|
| 1306 |
+
6
|
| 1307 |
+
6
|
| 1308 |
+
146
|
| 1309 |
+
2311
|
| 1310 |
+
6
|
| 1311 |
+
6
|
| 1312 |
+
18
|
| 1313 |
+
|
| 1314 |
+
Sr.No.
|
| 1315 |
+
p
|
| 1316 |
+
k
|
| 1317 |
+
m
|
| 1318 |
+
147
|
| 1319 |
+
2381
|
| 1320 |
+
2
|
| 1321 |
+
8
|
| 1322 |
+
148
|
| 1323 |
+
2591
|
| 1324 |
+
2
|
| 1325 |
+
7
|
| 1326 |
+
149
|
| 1327 |
+
2713
|
| 1328 |
+
6
|
| 1329 |
+
6
|
| 1330 |
+
150
|
| 1331 |
+
2731
|
| 1332 |
+
6
|
| 1333 |
+
7
|
| 1334 |
+
151
|
| 1335 |
+
2791
|
| 1336 |
+
6
|
| 1337 |
+
7
|
| 1338 |
+
152
|
| 1339 |
+
2887
|
| 1340 |
+
6
|
| 1341 |
+
6
|
| 1342 |
+
153
|
| 1343 |
+
2971
|
| 1344 |
+
6
|
| 1345 |
+
6
|
| 1346 |
+
154
|
| 1347 |
+
3041
|
| 1348 |
+
2
|
| 1349 |
+
7
|
| 1350 |
+
155
|
| 1351 |
+
3083
|
| 1352 |
+
2
|
| 1353 |
+
7
|
| 1354 |
+
156
|
| 1355 |
+
3191
|
| 1356 |
+
2
|
| 1357 |
+
7
|
| 1358 |
+
157
|
| 1359 |
+
3221
|
| 1360 |
+
2
|
| 1361 |
+
7
|
| 1362 |
+
158
|
| 1363 |
+
3229
|
| 1364 |
+
6
|
| 1365 |
+
6
|
| 1366 |
+
159
|
| 1367 |
+
3271
|
| 1368 |
+
6
|
| 1369 |
+
6
|
| 1370 |
+
160
|
| 1371 |
+
3301
|
| 1372 |
+
6
|
| 1373 |
+
7
|
| 1374 |
+
161
|
| 1375 |
+
3307
|
| 1376 |
+
6
|
| 1377 |
+
6
|
| 1378 |
+
162
|
| 1379 |
+
3313
|
| 1380 |
+
6
|
| 1381 |
+
6
|
| 1382 |
+
163
|
| 1383 |
+
3499
|
| 1384 |
+
6
|
| 1385 |
+
8
|
| 1386 |
+
164
|
| 1387 |
+
3547
|
| 1388 |
+
6
|
| 1389 |
+
8
|
| 1390 |
+
165
|
| 1391 |
+
3571
|
| 1392 |
+
6
|
| 1393 |
+
6
|
| 1394 |
+
166
|
| 1395 |
+
3739
|
| 1396 |
+
6
|
| 1397 |
+
6
|
| 1398 |
+
167
|
| 1399 |
+
3851
|
| 1400 |
+
2
|
| 1401 |
+
7
|
| 1402 |
+
168
|
| 1403 |
+
3911
|
| 1404 |
+
2
|
| 1405 |
+
7
|
| 1406 |
+
169
|
| 1407 |
+
4013
|
| 1408 |
+
27
|
| 1409 |
+
7
|
| 1410 |
+
170
|
| 1411 |
+
4159
|
| 1412 |
+
6
|
| 1413 |
+
6
|
| 1414 |
+
171
|
| 1415 |
+
4219
|
| 1416 |
+
6
|
| 1417 |
+
7
|
| 1418 |
+
172
|
| 1419 |
+
4241
|
| 1420 |
+
2
|
| 1421 |
+
7
|
| 1422 |
+
173
|
| 1423 |
+
4243
|
| 1424 |
+
6
|
| 1425 |
+
7
|
| 1426 |
+
174
|
| 1427 |
+
4261
|
| 1428 |
+
6
|
| 1429 |
+
6
|
| 1430 |
+
175
|
| 1431 |
+
4327
|
| 1432 |
+
6
|
| 1433 |
+
7
|
| 1434 |
+
176
|
| 1435 |
+
4421
|
| 1436 |
+
2
|
| 1437 |
+
7
|
| 1438 |
+
177
|
| 1439 |
+
4423
|
| 1440 |
+
6
|
| 1441 |
+
6
|
| 1442 |
+
178
|
| 1443 |
+
4567
|
| 1444 |
+
6
|
| 1445 |
+
6
|
| 1446 |
+
179
|
| 1447 |
+
4621
|
| 1448 |
+
6
|
| 1449 |
+
6
|
| 1450 |
+
180
|
| 1451 |
+
4663
|
| 1452 |
+
6
|
| 1453 |
+
6
|
| 1454 |
+
181
|
| 1455 |
+
4691
|
| 1456 |
+
2
|
| 1457 |
+
7
|
| 1458 |
+
182
|
| 1459 |
+
4751
|
| 1460 |
+
2
|
| 1461 |
+
7
|
| 1462 |
+
183
|
| 1463 |
+
4957
|
| 1464 |
+
6
|
| 1465 |
+
7
|
| 1466 |
+
184
|
| 1467 |
+
5419
|
| 1468 |
+
6
|
| 1469 |
+
7
|
| 1470 |
+
185
|
| 1471 |
+
5923
|
| 1472 |
+
6
|
| 1473 |
+
7
|
| 1474 |
+
186
|
| 1475 |
+
5981
|
| 1476 |
+
2
|
| 1477 |
+
8
|
| 1478 |
+
187
|
| 1479 |
+
6067
|
| 1480 |
+
6
|
| 1481 |
+
7
|
| 1482 |
+
188
|
| 1483 |
+
6211
|
| 1484 |
+
6
|
| 1485 |
+
7
|
| 1486 |
+
189
|
| 1487 |
+
6491
|
| 1488 |
+
2
|
| 1489 |
+
8
|
| 1490 |
+
Sr.No.
|
| 1491 |
+
p
|
| 1492 |
+
k
|
| 1493 |
+
m
|
| 1494 |
+
190
|
| 1495 |
+
6577
|
| 1496 |
+
6
|
| 1497 |
+
7
|
| 1498 |
+
191
|
| 1499 |
+
7159
|
| 1500 |
+
6
|
| 1501 |
+
7
|
| 1502 |
+
192
|
| 1503 |
+
7759
|
| 1504 |
+
6
|
| 1505 |
+
8
|
| 1506 |
+
193
|
| 1507 |
+
8009
|
| 1508 |
+
2
|
| 1509 |
+
9
|
| 1510 |
+
194
|
| 1511 |
+
8053
|
| 1512 |
+
6
|
| 1513 |
+
9
|
| 1514 |
+
195
|
| 1515 |
+
8191
|
| 1516 |
+
6
|
| 1517 |
+
7
|
| 1518 |
+
196
|
| 1519 |
+
8807
|
| 1520 |
+
2
|
| 1521 |
+
8
|
| 1522 |
+
197
|
| 1523 |
+
9103
|
| 1524 |
+
6
|
| 1525 |
+
7
|
| 1526 |
+
198
|
| 1527 |
+
9403
|
| 1528 |
+
6
|
| 1529 |
+
7
|
| 1530 |
+
199
|
| 1531 |
+
9421
|
| 1532 |
+
6
|
| 1533 |
+
7
|
| 1534 |
+
200
|
| 1535 |
+
9463
|
| 1536 |
+
6
|
| 1537 |
+
7
|
| 1538 |
+
201
|
| 1539 |
+
9719
|
| 1540 |
+
2
|
| 1541 |
+
8
|
| 1542 |
+
202
|
| 1543 |
+
9767
|
| 1544 |
+
2
|
| 1545 |
+
8
|
| 1546 |
+
203
|
| 1547 |
+
9871
|
| 1548 |
+
6
|
| 1549 |
+
7
|
| 1550 |
+
204
|
| 1551 |
+
9901
|
| 1552 |
+
6
|
| 1553 |
+
7
|
| 1554 |
+
205
|
| 1555 |
+
9967
|
| 1556 |
+
6
|
| 1557 |
+
7
|
| 1558 |
+
206
|
| 1559 |
+
10427
|
| 1560 |
+
2
|
| 1561 |
+
8
|
| 1562 |
+
207
|
| 1563 |
+
10949
|
| 1564 |
+
2
|
| 1565 |
+
10
|
| 1566 |
+
208
|
| 1567 |
+
10957
|
| 1568 |
+
6
|
| 1569 |
+
8
|
| 1570 |
+
209
|
| 1571 |
+
10979
|
| 1572 |
+
2
|
| 1573 |
+
8
|
| 1574 |
+
210
|
| 1575 |
+
11311
|
| 1576 |
+
6
|
| 1577 |
+
7
|
| 1578 |
+
211
|
| 1579 |
+
11593
|
| 1580 |
+
6
|
| 1581 |
+
7
|
| 1582 |
+
212
|
| 1583 |
+
11621
|
| 1584 |
+
2
|
| 1585 |
+
8
|
| 1586 |
+
213
|
| 1587 |
+
12959
|
| 1588 |
+
2
|
| 1589 |
+
9
|
| 1590 |
+
214
|
| 1591 |
+
14232
|
| 1592 |
+
6
|
| 1593 |
+
8
|
| 1594 |
+
215
|
| 1595 |
+
15313
|
| 1596 |
+
6
|
| 1597 |
+
8
|
| 1598 |
+
216
|
| 1599 |
+
15511
|
| 1600 |
+
6
|
| 1601 |
+
8
|
| 1602 |
+
217
|
| 1603 |
+
16381
|
| 1604 |
+
6
|
| 1605 |
+
8
|
| 1606 |
+
218
|
| 1607 |
+
17431
|
| 1608 |
+
6
|
| 1609 |
+
9
|
| 1610 |
+
219
|
| 1611 |
+
17491
|
| 1612 |
+
6
|
| 1613 |
+
9
|
| 1614 |
+
220
|
| 1615 |
+
19483
|
| 1616 |
+
6
|
| 1617 |
+
8
|
| 1618 |
+
221
|
| 1619 |
+
19687
|
| 1620 |
+
6
|
| 1621 |
+
8
|
| 1622 |
+
222
|
| 1623 |
+
19891
|
| 1624 |
+
6
|
| 1625 |
+
8
|
| 1626 |
+
223
|
| 1627 |
+
20011
|
| 1628 |
+
6
|
| 1629 |
+
8
|
| 1630 |
+
224
|
| 1631 |
+
20441
|
| 1632 |
+
2
|
| 1633 |
+
10
|
| 1634 |
+
225
|
| 1635 |
+
21391
|
| 1636 |
+
6
|
| 1637 |
+
8
|
| 1638 |
+
226
|
| 1639 |
+
22543
|
| 1640 |
+
6
|
| 1641 |
+
8
|
| 1642 |
+
227
|
| 1643 |
+
23143
|
| 1644 |
+
6
|
| 1645 |
+
8
|
| 1646 |
+
228
|
| 1647 |
+
23671
|
| 1648 |
+
6
|
| 1649 |
+
9
|
| 1650 |
+
229
|
| 1651 |
+
24181
|
| 1652 |
+
6
|
| 1653 |
+
8
|
| 1654 |
+
230
|
| 1655 |
+
24683
|
| 1656 |
+
2
|
| 1657 |
+
9
|
| 1658 |
+
231
|
| 1659 |
+
25171
|
| 1660 |
+
6
|
| 1661 |
+
9
|
| 1662 |
+
232
|
| 1663 |
+
25411
|
| 1664 |
+
6
|
| 1665 |
+
8
|
| 1666 |
+
19
|
| 1667 |
+
|
| 1668 |
+
for t=8:
|
| 1669 |
+
Sr.No.
|
| 1670 |
+
p
|
| 1671 |
+
k
|
| 1672 |
+
m
|
| 1673 |
+
1
|
| 1674 |
+
64
|
| 1675 |
+
6
|
| 1676 |
+
7
|
| 1677 |
+
2
|
| 1678 |
+
128
|
| 1679 |
+
3
|
| 1680 |
+
6
|
| 1681 |
+
3
|
| 1682 |
+
256
|
| 1683 |
+
3
|
| 1684 |
+
6
|
| 1685 |
+
4
|
| 1686 |
+
512
|
| 1687 |
+
6
|
| 1688 |
+
10
|
| 1689 |
+
5
|
| 1690 |
+
1024
|
| 1691 |
+
3
|
| 1692 |
+
8
|
| 1693 |
+
6
|
| 1694 |
+
81
|
| 1695 |
+
2
|
| 1696 |
+
5
|
| 1697 |
+
7
|
| 1698 |
+
243
|
| 1699 |
+
2
|
| 1700 |
+
6
|
| 1701 |
+
8
|
| 1702 |
+
125
|
| 1703 |
+
6
|
| 1704 |
+
6
|
| 1705 |
+
9
|
| 1706 |
+
49
|
| 1707 |
+
6
|
| 1708 |
+
4
|
| 1709 |
+
10
|
| 1710 |
+
343
|
| 1711 |
+
6
|
| 1712 |
+
9
|
| 1713 |
+
11
|
| 1714 |
+
121
|
| 1715 |
+
6
|
| 1716 |
+
5
|
| 1717 |
+
12
|
| 1718 |
+
169
|
| 1719 |
+
6
|
| 1720 |
+
5
|
| 1721 |
+
13
|
| 1722 |
+
361
|
| 1723 |
+
6
|
| 1724 |
+
6
|
| 1725 |
+
14
|
| 1726 |
+
529
|
| 1727 |
+
6
|
| 1728 |
+
7
|
| 1729 |
+
15
|
| 1730 |
+
841
|
| 1731 |
+
6
|
| 1732 |
+
7
|
| 1733 |
+
16
|
| 1734 |
+
961
|
| 1735 |
+
6
|
| 1736 |
+
7
|
| 1737 |
+
17
|
| 1738 |
+
53
|
| 1739 |
+
6
|
| 1740 |
+
5
|
| 1741 |
+
18
|
| 1742 |
+
59
|
| 1743 |
+
6
|
| 1744 |
+
6
|
| 1745 |
+
19
|
| 1746 |
+
61
|
| 1747 |
+
6
|
| 1748 |
+
4
|
| 1749 |
+
20
|
| 1750 |
+
67
|
| 1751 |
+
6
|
| 1752 |
+
6
|
| 1753 |
+
21
|
| 1754 |
+
71
|
| 1755 |
+
6
|
| 1756 |
+
4
|
| 1757 |
+
22
|
| 1758 |
+
73
|
| 1759 |
+
6
|
| 1760 |
+
5
|
| 1761 |
+
23
|
| 1762 |
+
79
|
| 1763 |
+
6
|
| 1764 |
+
6
|
| 1765 |
+
24
|
| 1766 |
+
89
|
| 1767 |
+
6
|
| 1768 |
+
6
|
| 1769 |
+
25
|
| 1770 |
+
97
|
| 1771 |
+
6
|
| 1772 |
+
5
|
| 1773 |
+
26
|
| 1774 |
+
101
|
| 1775 |
+
6
|
| 1776 |
+
5
|
| 1777 |
+
27
|
| 1778 |
+
103
|
| 1779 |
+
6
|
| 1780 |
+
5
|
| 1781 |
+
28
|
| 1782 |
+
107
|
| 1783 |
+
6
|
| 1784 |
+
5
|
| 1785 |
+
29
|
| 1786 |
+
109
|
| 1787 |
+
6
|
| 1788 |
+
6
|
| 1789 |
+
30
|
| 1790 |
+
113
|
| 1791 |
+
6
|
| 1792 |
+
5
|
| 1793 |
+
31
|
| 1794 |
+
127
|
| 1795 |
+
6
|
| 1796 |
+
6
|
| 1797 |
+
32
|
| 1798 |
+
131
|
| 1799 |
+
6
|
| 1800 |
+
6
|
| 1801 |
+
33
|
| 1802 |
+
137
|
| 1803 |
+
6
|
| 1804 |
+
7
|
| 1805 |
+
34
|
| 1806 |
+
139
|
| 1807 |
+
6
|
| 1808 |
+
6
|
| 1809 |
+
35
|
| 1810 |
+
149
|
| 1811 |
+
6
|
| 1812 |
+
6
|
| 1813 |
+
36
|
| 1814 |
+
151
|
| 1815 |
+
6
|
| 1816 |
+
6
|
| 1817 |
+
37
|
| 1818 |
+
157
|
| 1819 |
+
6
|
| 1820 |
+
7
|
| 1821 |
+
38
|
| 1822 |
+
163
|
| 1823 |
+
6
|
| 1824 |
+
5
|
| 1825 |
+
Sr.No.
|
| 1826 |
+
p
|
| 1827 |
+
k
|
| 1828 |
+
m
|
| 1829 |
+
39
|
| 1830 |
+
167
|
| 1831 |
+
6
|
| 1832 |
+
6
|
| 1833 |
+
40
|
| 1834 |
+
173
|
| 1835 |
+
6
|
| 1836 |
+
7
|
| 1837 |
+
41
|
| 1838 |
+
179
|
| 1839 |
+
6
|
| 1840 |
+
6
|
| 1841 |
+
42
|
| 1842 |
+
181
|
| 1843 |
+
6
|
| 1844 |
+
6
|
| 1845 |
+
43
|
| 1846 |
+
191
|
| 1847 |
+
6
|
| 1848 |
+
7
|
| 1849 |
+
44
|
| 1850 |
+
197
|
| 1851 |
+
6
|
| 1852 |
+
6
|
| 1853 |
+
45
|
| 1854 |
+
211
|
| 1855 |
+
6
|
| 1856 |
+
7
|
| 1857 |
+
46
|
| 1858 |
+
223
|
| 1859 |
+
6
|
| 1860 |
+
7
|
| 1861 |
+
47
|
| 1862 |
+
227
|
| 1863 |
+
6
|
| 1864 |
+
7
|
| 1865 |
+
48
|
| 1866 |
+
229
|
| 1867 |
+
6
|
| 1868 |
+
8
|
| 1869 |
+
49
|
| 1870 |
+
233
|
| 1871 |
+
6
|
| 1872 |
+
8
|
| 1873 |
+
50
|
| 1874 |
+
239
|
| 1875 |
+
6
|
| 1876 |
+
7
|
| 1877 |
+
51
|
| 1878 |
+
241
|
| 1879 |
+
6
|
| 1880 |
+
7
|
| 1881 |
+
52
|
| 1882 |
+
251
|
| 1883 |
+
6
|
| 1884 |
+
5
|
| 1885 |
+
53
|
| 1886 |
+
257
|
| 1887 |
+
6
|
| 1888 |
+
5
|
| 1889 |
+
54
|
| 1890 |
+
263
|
| 1891 |
+
6
|
| 1892 |
+
7
|
| 1893 |
+
55
|
| 1894 |
+
269
|
| 1895 |
+
6
|
| 1896 |
+
6
|
| 1897 |
+
56
|
| 1898 |
+
271
|
| 1899 |
+
6
|
| 1900 |
+
6
|
| 1901 |
+
57
|
| 1902 |
+
277
|
| 1903 |
+
6
|
| 1904 |
+
6
|
| 1905 |
+
58
|
| 1906 |
+
283
|
| 1907 |
+
6
|
| 1908 |
+
6
|
| 1909 |
+
59
|
| 1910 |
+
293
|
| 1911 |
+
6
|
| 1912 |
+
7
|
| 1913 |
+
60
|
| 1914 |
+
311
|
| 1915 |
+
6
|
| 1916 |
+
7
|
| 1917 |
+
61
|
| 1918 |
+
313
|
| 1919 |
+
6
|
| 1920 |
+
6
|
| 1921 |
+
62
|
| 1922 |
+
317
|
| 1923 |
+
6
|
| 1924 |
+
6
|
| 1925 |
+
63
|
| 1926 |
+
331
|
| 1927 |
+
6
|
| 1928 |
+
8
|
| 1929 |
+
64
|
| 1930 |
+
337
|
| 1931 |
+
6
|
| 1932 |
+
6
|
| 1933 |
+
65
|
| 1934 |
+
347
|
| 1935 |
+
6
|
| 1936 |
+
6
|
| 1937 |
+
66
|
| 1938 |
+
349
|
| 1939 |
+
6
|
| 1940 |
+
6
|
| 1941 |
+
67
|
| 1942 |
+
353
|
| 1943 |
+
6
|
| 1944 |
+
6
|
| 1945 |
+
68
|
| 1946 |
+
359
|
| 1947 |
+
6
|
| 1948 |
+
7
|
| 1949 |
+
69
|
| 1950 |
+
367
|
| 1951 |
+
6
|
| 1952 |
+
6
|
| 1953 |
+
70
|
| 1954 |
+
373
|
| 1955 |
+
6
|
| 1956 |
+
7
|
| 1957 |
+
71
|
| 1958 |
+
379
|
| 1959 |
+
6
|
| 1960 |
+
6
|
| 1961 |
+
72
|
| 1962 |
+
383
|
| 1963 |
+
6
|
| 1964 |
+
7
|
| 1965 |
+
73
|
| 1966 |
+
389
|
| 1967 |
+
6
|
| 1968 |
+
8
|
| 1969 |
+
74
|
| 1970 |
+
397
|
| 1971 |
+
6
|
| 1972 |
+
6
|
| 1973 |
+
75
|
| 1974 |
+
401
|
| 1975 |
+
6
|
| 1976 |
+
8
|
| 1977 |
+
76
|
| 1978 |
+
409
|
| 1979 |
+
6
|
| 1980 |
+
6
|
| 1981 |
+
20
|
| 1982 |
+
|
| 1983 |
+
Sr.No.
|
| 1984 |
+
p
|
| 1985 |
+
k
|
| 1986 |
+
m
|
| 1987 |
+
77
|
| 1988 |
+
433
|
| 1989 |
+
6
|
| 1990 |
+
7
|
| 1991 |
+
78
|
| 1992 |
+
439
|
| 1993 |
+
6
|
| 1994 |
+
7
|
| 1995 |
+
79
|
| 1996 |
+
443
|
| 1997 |
+
6
|
| 1998 |
+
7
|
| 1999 |
+
80
|
| 2000 |
+
457
|
| 2001 |
+
6
|
| 2002 |
+
7
|
| 2003 |
+
81
|
| 2004 |
+
467
|
| 2005 |
+
6
|
| 2006 |
+
7
|
| 2007 |
+
82
|
| 2008 |
+
491
|
| 2009 |
+
6
|
| 2010 |
+
7
|
| 2011 |
+
83
|
| 2012 |
+
499
|
| 2013 |
+
6
|
| 2014 |
+
8
|
| 2015 |
+
84
|
| 2016 |
+
509
|
| 2017 |
+
6
|
| 2018 |
+
7
|
| 2019 |
+
85
|
| 2020 |
+
521
|
| 2021 |
+
6
|
| 2022 |
+
7
|
| 2023 |
+
86
|
| 2024 |
+
523
|
| 2025 |
+
6
|
| 2026 |
+
6
|
| 2027 |
+
87
|
| 2028 |
+
541
|
| 2029 |
+
6
|
| 2030 |
+
6
|
| 2031 |
+
88
|
| 2032 |
+
547
|
| 2033 |
+
6
|
| 2034 |
+
8
|
| 2035 |
+
89
|
| 2036 |
+
557
|
| 2037 |
+
6
|
| 2038 |
+
7
|
| 2039 |
+
90
|
| 2040 |
+
563
|
| 2041 |
+
6
|
| 2042 |
+
9
|
| 2043 |
+
91
|
| 2044 |
+
569
|
| 2045 |
+
6
|
| 2046 |
+
6
|
| 2047 |
+
92
|
| 2048 |
+
571
|
| 2049 |
+
6
|
| 2050 |
+
9
|
| 2051 |
+
93
|
| 2052 |
+
587
|
| 2053 |
+
6
|
| 2054 |
+
7
|
| 2055 |
+
94
|
| 2056 |
+
593
|
| 2057 |
+
6
|
| 2058 |
+
8
|
| 2059 |
+
95
|
| 2060 |
+
599
|
| 2061 |
+
6
|
| 2062 |
+
8
|
| 2063 |
+
96
|
| 2064 |
+
601
|
| 2065 |
+
6
|
| 2066 |
+
7
|
| 2067 |
+
97
|
| 2068 |
+
617
|
| 2069 |
+
6
|
| 2070 |
+
8
|
| 2071 |
+
98
|
| 2072 |
+
619
|
| 2073 |
+
6
|
| 2074 |
+
7
|
| 2075 |
+
99
|
| 2076 |
+
631
|
| 2077 |
+
6
|
| 2078 |
+
7
|
| 2079 |
+
100
|
| 2080 |
+
647
|
| 2081 |
+
6
|
| 2082 |
+
7
|
| 2083 |
+
101
|
| 2084 |
+
653
|
| 2085 |
+
6
|
| 2086 |
+
7
|
| 2087 |
+
102
|
| 2088 |
+
661
|
| 2089 |
+
6
|
| 2090 |
+
7
|
| 2091 |
+
103
|
| 2092 |
+
683
|
| 2093 |
+
6
|
| 2094 |
+
7
|
| 2095 |
+
104
|
| 2096 |
+
691
|
| 2097 |
+
6
|
| 2098 |
+
7
|
| 2099 |
+
105
|
| 2100 |
+
701
|
| 2101 |
+
6
|
| 2102 |
+
7
|
| 2103 |
+
106
|
| 2104 |
+
709
|
| 2105 |
+
6
|
| 2106 |
+
7
|
| 2107 |
+
107
|
| 2108 |
+
733
|
| 2109 |
+
6
|
| 2110 |
+
7
|
| 2111 |
+
108
|
| 2112 |
+
739
|
| 2113 |
+
6
|
| 2114 |
+
7
|
| 2115 |
+
109
|
| 2116 |
+
743
|
| 2117 |
+
6
|
| 2118 |
+
9
|
| 2119 |
+
110
|
| 2120 |
+
757
|
| 2121 |
+
6
|
| 2122 |
+
8
|
| 2123 |
+
111
|
| 2124 |
+
773
|
| 2125 |
+
6
|
| 2126 |
+
8
|
| 2127 |
+
112
|
| 2128 |
+
787
|
| 2129 |
+
6
|
| 2130 |
+
8
|
| 2131 |
+
113
|
| 2132 |
+
797
|
| 2133 |
+
6
|
| 2134 |
+
8
|
| 2135 |
+
114
|
| 2136 |
+
809
|
| 2137 |
+
6
|
| 2138 |
+
8
|
| 2139 |
+
Sr.No.
|
| 2140 |
+
p
|
| 2141 |
+
k
|
| 2142 |
+
m
|
| 2143 |
+
115
|
| 2144 |
+
811
|
| 2145 |
+
6
|
| 2146 |
+
7
|
| 2147 |
+
116
|
| 2148 |
+
823
|
| 2149 |
+
6
|
| 2150 |
+
8
|
| 2151 |
+
117
|
| 2152 |
+
827
|
| 2153 |
+
6
|
| 2154 |
+
8
|
| 2155 |
+
118
|
| 2156 |
+
829
|
| 2157 |
+
6
|
| 2158 |
+
7
|
| 2159 |
+
119
|
| 2160 |
+
839
|
| 2161 |
+
6
|
| 2162 |
+
7
|
| 2163 |
+
120
|
| 2164 |
+
857
|
| 2165 |
+
6
|
| 2166 |
+
7
|
| 2167 |
+
121
|
| 2168 |
+
859
|
| 2169 |
+
6
|
| 2170 |
+
8
|
| 2171 |
+
122
|
| 2172 |
+
863
|
| 2173 |
+
6
|
| 2174 |
+
8
|
| 2175 |
+
123
|
| 2176 |
+
881
|
| 2177 |
+
6
|
| 2178 |
+
7
|
| 2179 |
+
124
|
| 2180 |
+
887
|
| 2181 |
+
6
|
| 2182 |
+
7
|
| 2183 |
+
125
|
| 2184 |
+
919
|
| 2185 |
+
76
|
| 2186 |
+
7
|
| 2187 |
+
126
|
| 2188 |
+
929
|
| 2189 |
+
6
|
| 2190 |
+
7
|
| 2191 |
+
127
|
| 2192 |
+
941
|
| 2193 |
+
6
|
| 2194 |
+
7
|
| 2195 |
+
128
|
| 2196 |
+
947
|
| 2197 |
+
6
|
| 2198 |
+
8
|
| 2199 |
+
129
|
| 2200 |
+
953
|
| 2201 |
+
6
|
| 2202 |
+
7
|
| 2203 |
+
130
|
| 2204 |
+
971
|
| 2205 |
+
6
|
| 2206 |
+
8
|
| 2207 |
+
131
|
| 2208 |
+
977
|
| 2209 |
+
6
|
| 2210 |
+
8
|
| 2211 |
+
132
|
| 2212 |
+
983
|
| 2213 |
+
6
|
| 2214 |
+
7
|
| 2215 |
+
133
|
| 2216 |
+
991
|
| 2217 |
+
6
|
| 2218 |
+
7
|
| 2219 |
+
134
|
| 2220 |
+
1009
|
| 2221 |
+
6
|
| 2222 |
+
7
|
| 2223 |
+
135
|
| 2224 |
+
1013
|
| 2225 |
+
6
|
| 2226 |
+
7
|
| 2227 |
+
136
|
| 2228 |
+
1021
|
| 2229 |
+
6
|
| 2230 |
+
8
|
| 2231 |
+
137
|
| 2232 |
+
1033
|
| 2233 |
+
6
|
| 2234 |
+
8
|
| 2235 |
+
138
|
| 2236 |
+
1039
|
| 2237 |
+
6
|
| 2238 |
+
8
|
| 2239 |
+
139
|
| 2240 |
+
1061
|
| 2241 |
+
6
|
| 2242 |
+
9
|
| 2243 |
+
140
|
| 2244 |
+
1063
|
| 2245 |
+
6
|
| 2246 |
+
8
|
| 2247 |
+
141
|
| 2248 |
+
1069
|
| 2249 |
+
6
|
| 2250 |
+
7
|
| 2251 |
+
142
|
| 2252 |
+
1087
|
| 2253 |
+
6
|
| 2254 |
+
7
|
| 2255 |
+
143
|
| 2256 |
+
1091
|
| 2257 |
+
6
|
| 2258 |
+
8
|
| 2259 |
+
144
|
| 2260 |
+
1093
|
| 2261 |
+
6
|
| 2262 |
+
7
|
| 2263 |
+
145
|
| 2264 |
+
1097
|
| 2265 |
+
6
|
| 2266 |
+
8
|
| 2267 |
+
146
|
| 2268 |
+
1103
|
| 2269 |
+
6
|
| 2270 |
+
8
|
| 2271 |
+
147
|
| 2272 |
+
1109
|
| 2273 |
+
6
|
| 2274 |
+
8
|
| 2275 |
+
148
|
| 2276 |
+
1117
|
| 2277 |
+
6
|
| 2278 |
+
8
|
| 2279 |
+
149
|
| 2280 |
+
1123
|
| 2281 |
+
6
|
| 2282 |
+
8
|
| 2283 |
+
150
|
| 2284 |
+
1201
|
| 2285 |
+
6
|
| 2286 |
+
9
|
| 2287 |
+
151
|
| 2288 |
+
1213
|
| 2289 |
+
6
|
| 2290 |
+
8
|
| 2291 |
+
152
|
| 2292 |
+
1223
|
| 2293 |
+
6
|
| 2294 |
+
9
|
| 2295 |
+
21
|
| 2296 |
+
|
| 2297 |
+
Sr.No.
|
| 2298 |
+
p
|
| 2299 |
+
k
|
| 2300 |
+
m
|
| 2301 |
+
153
|
| 2302 |
+
1231
|
| 2303 |
+
6
|
| 2304 |
+
8
|
| 2305 |
+
154
|
| 2306 |
+
1277
|
| 2307 |
+
6
|
| 2308 |
+
9
|
| 2309 |
+
155
|
| 2310 |
+
1279
|
| 2311 |
+
6
|
| 2312 |
+
8
|
| 2313 |
+
156
|
| 2314 |
+
1283
|
| 2315 |
+
6
|
| 2316 |
+
9
|
| 2317 |
+
157
|
| 2318 |
+
1289
|
| 2319 |
+
6
|
| 2320 |
+
9
|
| 2321 |
+
158
|
| 2322 |
+
1291
|
| 2323 |
+
6
|
| 2324 |
+
9
|
| 2325 |
+
159
|
| 2326 |
+
1303
|
| 2327 |
+
6
|
| 2328 |
+
8
|
| 2329 |
+
160
|
| 2330 |
+
1319
|
| 2331 |
+
6
|
| 2332 |
+
8
|
| 2333 |
+
161
|
| 2334 |
+
1321
|
| 2335 |
+
6
|
| 2336 |
+
8
|
| 2337 |
+
162
|
| 2338 |
+
191
|
| 2339 |
+
6
|
| 2340 |
+
7
|
| 2341 |
+
163
|
| 2342 |
+
911
|
| 2343 |
+
30
|
| 2344 |
+
9
|
| 2345 |
+
164
|
| 2346 |
+
659
|
| 2347 |
+
30
|
| 2348 |
+
8
|
| 2349 |
+
165
|
| 2350 |
+
1301
|
| 2351 |
+
30
|
| 2352 |
+
10
|
| 2353 |
+
Sr.No.
|
| 2354 |
+
p
|
| 2355 |
+
k
|
| 2356 |
+
m
|
| 2357 |
+
166
|
| 2358 |
+
281
|
| 2359 |
+
30
|
| 2360 |
+
6
|
| 2361 |
+
167
|
| 2362 |
+
410
|
| 2363 |
+
30
|
| 2364 |
+
6
|
| 2365 |
+
168
|
| 2366 |
+
421
|
| 2367 |
+
30
|
| 2368 |
+
8
|
| 2369 |
+
169
|
| 2370 |
+
937
|
| 2371 |
+
30
|
| 2372 |
+
7
|
| 2373 |
+
170
|
| 2374 |
+
1331
|
| 2375 |
+
30
|
| 2376 |
+
9
|
| 2377 |
+
171
|
| 2378 |
+
307
|
| 2379 |
+
30
|
| 2380 |
+
7
|
| 2381 |
+
172
|
| 2382 |
+
1217
|
| 2383 |
+
30
|
| 2384 |
+
7
|
| 2385 |
+
173
|
| 2386 |
+
967
|
| 2387 |
+
30
|
| 2388 |
+
8
|
| 2389 |
+
174
|
| 2390 |
+
461
|
| 2391 |
+
30
|
| 2392 |
+
7
|
| 2393 |
+
175
|
| 2394 |
+
463
|
| 2395 |
+
30
|
| 2396 |
+
7
|
| 2397 |
+
176
|
| 2398 |
+
853
|
| 2399 |
+
30
|
| 2400 |
+
9
|
| 2401 |
+
177
|
| 2402 |
+
727
|
| 2403 |
+
30
|
| 2404 |
+
7
|
| 2405 |
+
178
|
| 2406 |
+
729
|
| 2407 |
+
30
|
| 2408 |
+
9
|
| 2409 |
+
for t=9:
|
| 2410 |
+
Sr.No.
|
| 2411 |
+
p
|
| 2412 |
+
k
|
| 2413 |
+
m
|
| 2414 |
+
1
|
| 2415 |
+
8
|
| 2416 |
+
7
|
| 2417 |
+
2
|
| 2418 |
+
2
|
| 2419 |
+
32
|
| 2420 |
+
7
|
| 2421 |
+
5
|
| 2422 |
+
3
|
| 2423 |
+
27
|
| 2424 |
+
2
|
| 2425 |
+
5
|
| 2426 |
+
4
|
| 2427 |
+
81
|
| 2428 |
+
14
|
| 2429 |
+
7
|
| 2430 |
+
5
|
| 2431 |
+
25
|
| 2432 |
+
6
|
| 2433 |
+
5
|
| 2434 |
+
6
|
| 2435 |
+
125
|
| 2436 |
+
2
|
| 2437 |
+
7
|
| 2438 |
+
7
|
| 2439 |
+
49
|
| 2440 |
+
6
|
| 2441 |
+
5
|
| 2442 |
+
8
|
| 2443 |
+
121
|
| 2444 |
+
6
|
| 2445 |
+
6
|
| 2446 |
+
9
|
| 2447 |
+
13
|
| 2448 |
+
6
|
| 2449 |
+
2
|
| 2450 |
+
Sr.No.
|
| 2451 |
+
p
|
| 2452 |
+
k
|
| 2453 |
+
m
|
| 2454 |
+
10
|
| 2455 |
+
169
|
| 2456 |
+
6
|
| 2457 |
+
7
|
| 2458 |
+
11
|
| 2459 |
+
17
|
| 2460 |
+
2
|
| 2461 |
+
3
|
| 2462 |
+
12
|
| 2463 |
+
19
|
| 2464 |
+
6
|
| 2465 |
+
3
|
| 2466 |
+
13
|
| 2467 |
+
23
|
| 2468 |
+
2
|
| 2469 |
+
5
|
| 2470 |
+
14
|
| 2471 |
+
29
|
| 2472 |
+
2
|
| 2473 |
+
5
|
| 2474 |
+
15
|
| 2475 |
+
31
|
| 2476 |
+
6
|
| 2477 |
+
4
|
| 2478 |
+
16
|
| 2479 |
+
37
|
| 2480 |
+
6
|
| 2481 |
+
5
|
| 2482 |
+
17
|
| 2483 |
+
43
|
| 2484 |
+
6
|
| 2485 |
+
6
|
| 2486 |
+
18
|
| 2487 |
+
47
|
| 2488 |
+
2
|
| 2489 |
+
5
|
| 2490 |
+
Sr.No.
|
| 2491 |
+
p
|
| 2492 |
+
k
|
| 2493 |
+
m
|
| 2494 |
+
19
|
| 2495 |
+
53
|
| 2496 |
+
2
|
| 2497 |
+
7
|
| 2498 |
+
20
|
| 2499 |
+
61
|
| 2500 |
+
6
|
| 2501 |
+
5
|
| 2502 |
+
21
|
| 2503 |
+
79
|
| 2504 |
+
6
|
| 2505 |
+
5
|
| 2506 |
+
22
|
| 2507 |
+
83
|
| 2508 |
+
2
|
| 2509 |
+
6
|
| 2510 |
+
23
|
| 2511 |
+
137
|
| 2512 |
+
2
|
| 2513 |
+
7
|
| 2514 |
+
24
|
| 2515 |
+
139
|
| 2516 |
+
6
|
| 2517 |
+
6
|
| 2518 |
+
25
|
| 2519 |
+
149
|
| 2520 |
+
2
|
| 2521 |
+
7
|
| 2522 |
+
26
|
| 2523 |
+
157
|
| 2524 |
+
6
|
| 2525 |
+
6
|
| 2526 |
+
27
|
| 2527 |
+
211
|
| 2528 |
+
6
|
| 2529 |
+
7
|
| 2530 |
+
for t=10:
|
| 2531 |
+
Sr.No.
|
| 2532 |
+
p
|
| 2533 |
+
k
|
| 2534 |
+
m
|
| 2535 |
+
1
|
| 2536 |
+
8
|
| 2537 |
+
3
|
| 2538 |
+
5
|
| 2539 |
+
2
|
| 2540 |
+
16
|
| 2541 |
+
3
|
| 2542 |
+
6
|
| 2543 |
+
3
|
| 2544 |
+
32
|
| 2545 |
+
3
|
| 2546 |
+
6
|
| 2547 |
+
4
|
| 2548 |
+
64
|
| 2549 |
+
6
|
| 2550 |
+
9
|
| 2551 |
+
5
|
| 2552 |
+
9
|
| 2553 |
+
2
|
| 2554 |
+
4
|
| 2555 |
+
6
|
| 2556 |
+
27
|
| 2557 |
+
2
|
| 2558 |
+
7
|
| 2559 |
+
7
|
| 2560 |
+
25
|
| 2561 |
+
6
|
| 2562 |
+
6
|
| 2563 |
+
Sr.No.
|
| 2564 |
+
p
|
| 2565 |
+
k
|
| 2566 |
+
m
|
| 2567 |
+
8
|
| 2568 |
+
49
|
| 2569 |
+
6
|
| 2570 |
+
6
|
| 2571 |
+
9
|
| 2572 |
+
11
|
| 2573 |
+
6
|
| 2574 |
+
3
|
| 2575 |
+
10
|
| 2576 |
+
13
|
| 2577 |
+
6
|
| 2578 |
+
4
|
| 2579 |
+
11
|
| 2580 |
+
17
|
| 2581 |
+
6
|
| 2582 |
+
4
|
| 2583 |
+
12
|
| 2584 |
+
19
|
| 2585 |
+
6
|
| 2586 |
+
5
|
| 2587 |
+
13
|
| 2588 |
+
23
|
| 2589 |
+
6
|
| 2590 |
+
5
|
| 2591 |
+
14
|
| 2592 |
+
29
|
| 2593 |
+
6
|
| 2594 |
+
6
|
| 2595 |
+
Sr.No.
|
| 2596 |
+
p
|
| 2597 |
+
k
|
| 2598 |
+
m
|
| 2599 |
+
15
|
| 2600 |
+
31
|
| 2601 |
+
6
|
| 2602 |
+
5
|
| 2603 |
+
16
|
| 2604 |
+
37
|
| 2605 |
+
6
|
| 2606 |
+
5
|
| 2607 |
+
17
|
| 2608 |
+
41
|
| 2609 |
+
6
|
| 2610 |
+
6
|
| 2611 |
+
18
|
| 2612 |
+
53
|
| 2613 |
+
6
|
| 2614 |
+
6
|
| 2615 |
+
19
|
| 2616 |
+
59
|
| 2617 |
+
6
|
| 2618 |
+
7
|
| 2619 |
+
20
|
| 2620 |
+
61
|
| 2621 |
+
6
|
| 2622 |
+
6
|
| 2623 |
+
21
|
| 2624 |
+
67
|
| 2625 |
+
6
|
| 2626 |
+
6
|
| 2627 |
+
22
|
| 2628 |
+
|
| 2629 |
+
for t=11:
|
| 2630 |
+
Sr.No.
|
| 2631 |
+
p
|
| 2632 |
+
k
|
| 2633 |
+
m
|
| 2634 |
+
1
|
| 2635 |
+
16
|
| 2636 |
+
3
|
| 2637 |
+
6
|
| 2638 |
+
2
|
| 2639 |
+
9
|
| 2640 |
+
2
|
| 2641 |
+
4
|
| 2642 |
+
3
|
| 2643 |
+
7
|
| 2644 |
+
2
|
| 2645 |
+
3
|
| 2646 |
+
4
|
| 2647 |
+
13
|
| 2648 |
+
2
|
| 2649 |
+
5
|
| 2650 |
+
for t=12:
|
| 2651 |
+
Sr.No.
|
| 2652 |
+
p
|
| 2653 |
+
k
|
| 2654 |
+
m
|
| 2655 |
+
1
|
| 2656 |
+
8
|
| 2657 |
+
39
|
| 2658 |
+
6
|
| 2659 |
+
2
|
| 2660 |
+
16
|
| 2661 |
+
39
|
| 2662 |
+
7
|
| 2663 |
+
3
|
| 2664 |
+
32
|
| 2665 |
+
39
|
| 2666 |
+
9
|
| 2667 |
+
4
|
| 2668 |
+
9
|
| 2669 |
+
2
|
| 2670 |
+
6
|
| 2671 |
+
5
|
| 2672 |
+
13
|
| 2673 |
+
6
|
| 2674 |
+
6
|
| 2675 |
+
Sr.No.
|
| 2676 |
+
p
|
| 2677 |
+
k
|
| 2678 |
+
m
|
| 2679 |
+
6
|
| 2680 |
+
17
|
| 2681 |
+
6
|
| 2682 |
+
6
|
| 2683 |
+
7
|
| 2684 |
+
19
|
| 2685 |
+
6
|
| 2686 |
+
6
|
| 2687 |
+
8
|
| 2688 |
+
29
|
| 2689 |
+
6
|
| 2690 |
+
9
|
| 2691 |
+
9
|
| 2692 |
+
27
|
| 2693 |
+
30
|
| 2694 |
+
6
|
| 2695 |
+
Sr.No.
|
| 2696 |
+
p
|
| 2697 |
+
k
|
| 2698 |
+
m
|
| 2699 |
+
10
|
| 2700 |
+
11
|
| 2701 |
+
30
|
| 2702 |
+
6
|
| 2703 |
+
11
|
| 2704 |
+
23
|
| 2705 |
+
30
|
| 2706 |
+
7
|
| 2707 |
+
12
|
| 2708 |
+
31
|
| 2709 |
+
30
|
| 2710 |
+
6
|
| 2711 |
+
13
|
| 2712 |
+
37
|
| 2713 |
+
30
|
| 2714 |
+
8
|
| 2715 |
+
for t=14:
|
| 2716 |
+
Sr.No.
|
| 2717 |
+
p
|
| 2718 |
+
k
|
| 2719 |
+
m
|
| 2720 |
+
1
|
| 2721 |
+
4
|
| 2722 |
+
15
|
| 2723 |
+
4
|
| 2724 |
+
2
|
| 2725 |
+
5
|
| 2726 |
+
6
|
| 2727 |
+
3
|
| 2728 |
+
3
|
| 2729 |
+
7
|
| 2730 |
+
6
|
| 2731 |
+
4
|
| 2732 |
+
4
|
| 2733 |
+
3
|
| 2734 |
+
2
|
| 2735 |
+
2
|
| 2736 |
+
for t=15:
|
| 2737 |
+
Sr.No.
|
| 2738 |
+
p
|
| 2739 |
+
k
|
| 2740 |
+
m
|
| 2741 |
+
1
|
| 2742 |
+
4
|
| 2743 |
+
3
|
| 2744 |
+
5
|
| 2745 |
+
2
|
| 2746 |
+
3
|
| 2747 |
+
2
|
| 2748 |
+
3
|
| 2749 |
+
3
|
| 2750 |
+
9
|
| 2751 |
+
2
|
| 2752 |
+
7
|
| 2753 |
+
4
|
| 2754 |
+
5
|
| 2755 |
+
2
|
| 2756 |
+
5
|
| 2757 |
+
5
|
| 2758 |
+
16
|
| 2759 |
+
15
|
| 2760 |
+
9
|
| 2761 |
+
for t=16:
|
| 2762 |
+
Sr.No.
|
| 2763 |
+
p
|
| 2764 |
+
k
|
| 2765 |
+
m
|
| 2766 |
+
1
|
| 2767 |
+
4
|
| 2768 |
+
3
|
| 2769 |
+
4
|
| 2770 |
+
2
|
| 2771 |
+
8
|
| 2772 |
+
3
|
| 2773 |
+
8
|
| 2774 |
+
3
|
| 2775 |
+
3
|
| 2776 |
+
2
|
| 2777 |
+
4
|
| 2778 |
+
4
|
| 2779 |
+
5
|
| 2780 |
+
2
|
| 2781 |
+
5
|
| 2782 |
+
23
|
| 2783 |
+
|
| 2784 |
+
for t=18:
|
| 2785 |
+
Sr.No.
|
| 2786 |
+
p
|
| 2787 |
+
k
|
| 2788 |
+
m
|
| 2789 |
+
1
|
| 2790 |
+
3
|
| 2791 |
+
2
|
| 2792 |
+
5
|
| 2793 |
+
2
|
| 2794 |
+
4
|
| 2795 |
+
15
|
| 2796 |
+
6
|
| 2797 |
+
3
|
| 2798 |
+
5
|
| 2799 |
+
6
|
| 2800 |
+
5
|
| 2801 |
+
for t=20:
|
| 2802 |
+
Sr.No.
|
| 2803 |
+
p
|
| 2804 |
+
k
|
| 2805 |
+
m
|
| 2806 |
+
1
|
| 2807 |
+
4
|
| 2808 |
+
3
|
| 2809 |
+
6
|
| 2810 |
+
2
|
| 2811 |
+
8
|
| 2812 |
+
15
|
| 2813 |
+
9
|
| 2814 |
+
for t=22:
|
| 2815 |
+
Sr.No.
|
| 2816 |
+
p
|
| 2817 |
+
k
|
| 2818 |
+
m
|
| 2819 |
+
1
|
| 2820 |
+
2
|
| 2821 |
+
15
|
| 2822 |
+
2
|
| 2823 |
+
for t=24:
|
| 2824 |
+
Sr.No.
|
| 2825 |
+
p
|
| 2826 |
+
k
|
| 2827 |
+
m
|
| 2828 |
+
1
|
| 2829 |
+
4
|
| 2830 |
+
3
|
| 2831 |
+
8
|
| 2832 |
+
2
|
| 2833 |
+
3
|
| 2834 |
+
2
|
| 2835 |
+
6
|
| 2836 |
+
for t=28:
|
| 2837 |
+
Sr.No.
|
| 2838 |
+
p
|
| 2839 |
+
k
|
| 2840 |
+
m
|
| 2841 |
+
1
|
| 2842 |
+
2
|
| 2843 |
+
15
|
| 2844 |
+
4
|
| 2845 |
+
for t=30:
|
| 2846 |
+
Sr.No.
|
| 2847 |
+
p
|
| 2848 |
+
k
|
| 2849 |
+
m
|
| 2850 |
+
1
|
| 2851 |
+
2
|
| 2852 |
+
3
|
| 2853 |
+
5
|
| 2854 |
+
for t=36:
|
| 2855 |
+
Sr.No.
|
| 2856 |
+
p
|
| 2857 |
+
k
|
| 2858 |
+
m
|
| 2859 |
+
1
|
| 2860 |
+
2
|
| 2861 |
+
15
|
| 2862 |
+
6
|
| 2863 |
+
24
|
| 2864 |
+
|
2dE0T4oBgHgl3EQfdwCH/content/tmp_files/load_file.txt
ADDED
|
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See raw diff
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ADDED
|
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size 188953
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size 138261
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size 720941
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+
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ADDED
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+
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|
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|
|
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|
| 1 |
+
|
| 2 |
+
1
|
| 3 |
+
Giant resonant enhancement for photo-induced
|
| 4 |
+
superconductivity in K3C60
|
| 5 |
+
|
| 6 |
+
E. Rowe1,*, B. Yuan1, M. Buzzi1, G. Jotzu1, Y. Zhu1, M. Fechner1, M. Först1, B. Liu1,2
|
| 7 |
+
D. Pontiroli3, M. Riccò3, A. Cavalleri1,4,*
|
| 8 |
+
|
| 9 |
+
1 Max Planck Institute for the Structure and Dynamics of Matter, Hamburg, Germany
|
| 10 |
+
2 Paul Scherrer Institute, Villigen, Switzerland
|
| 11 |
+
3 Dipartimento di Scienze Matematiche, Fisiche e Informatiche, Università degli Studi di Parma, Italy
|
| 12 |
+
4 Department of Physics, Clarendon Laboratory, University of Oxford, United Kingdom
|
| 13 |
+
* e-mail: edward.rowe@mpsd.mpg.de, andrea.cavalleri@mpsd.mpg.de
|
| 14 |
+
|
| 15 |
+
Photo-excitation at terahertz and mid-infrared frequencies has emerged as a new
|
| 16 |
+
way to manipulate functionalities in quantum materials, in some cases creating
|
| 17 |
+
non-equilibrium phases that have no equilibrium analogue. In K3C60, a metastable
|
| 18 |
+
zero-resistance phase was documented with optical properties and pressure de-
|
| 19 |
+
pendences compatible with non-equilibrium high temperature superconductivity.
|
| 20 |
+
Here, we report the discovery of a dominant energy scale for this phenomenon,
|
| 21 |
+
along with the demonstration of a giant increase in photo-susceptibility near
|
| 22 |
+
10 THz excitation frequency. At these drive frequencies a metastable supercon-
|
| 23 |
+
ducting-like phase is observed up to room temperature for fluences as low as
|
| 24 |
+
~400 µJ/cm2. These findings shed light on the microscopic mechanism underlying
|
| 25 |
+
photo-induced superconductivity. They also trace a path towards steady state op-
|
| 26 |
+
eration, currently limited by the availability of a suitable high-repetition rate opti-
|
| 27 |
+
cal source at these frequencies.
|
| 28 |
+
|
| 29 |
+
|
| 30 |
+
|
| 31 |
+
|
| 32 |
+
2
|
| 33 |
+
The search for new non-equilibrium functional phases in quantum materials, such as op-
|
| 34 |
+
tically induced ferroelectricity1,2, magnetism3-5, charge density wave order6,7, non-trivial
|
| 35 |
+
topology8,9 and superconductivity10-18, has become a central research theme in condensed
|
| 36 |
+
matter physics. In the case of K3C60 (Fig. 1a), mid infrared optical pulses have been exten-
|
| 37 |
+
sively documented to yield an unconventional non-equilibrium phase which exhibits met-
|
| 38 |
+
astable zero-resistance14, an extraordinarily high mobility and a superconducting-like gap
|
| 39 |
+
in the optical conductivity12,14 that reduce with applied pressure13, and nonlinear I-V char-
|
| 40 |
+
acteristics19. All these observations are indicative of non-equilibrium high temperature
|
| 41 |
+
superconductivity, observed at base temperatures far exceeding the highest equilibrium
|
| 42 |
+
superconducting critical temperature of any alkali-doped fulleride (Fig. 1b).
|
| 43 |
+
Typical experimental results reported to date are displayed in Fig. 2c. K3C60 powders were
|
| 44 |
+
held at a base temperature T = 100 K ≫ T! = 20 K and irradiated with 1 ps-long pulses
|
| 45 |
+
with 170 meV photon energy (l ~ 7.3 µm, ) ~ 41 THz) at a fluence of 18 mJ/cm². This
|
| 46 |
+
strong excitation regime yielded a long-lived transient state with dramatic changes in
|
| 47 |
+
both the real and imaginary parts of the optical conductivity, measured using phase
|
| 48 |
+
|
| 49 |
+
Figure 1. Crystal structure and phase diagram K3C60. (a) Crystal structure of the organic molec-
|
| 50 |
+
ular solid K3C60. C60 molecules are situated at the vertices of a face-centered-cubic lattice. Potassium
|
| 51 |
+
atoms (red) occupy the interstitial voids. (b) Pressure-temperature phase diagram of the fcc-A3C60
|
| 52 |
+
alkali-doped fulleride family of compounds. Physical pressure tunes the spacing between the C60
|
| 53 |
+
molecules. The grey line indicates the boundary between the insulating and metallic/superconduct-
|
| 54 |
+
ing compounds. The blue shaded area indicates where superconductivity is observed at equilibrium.
|
| 55 |
+
The star indicates the K3C60 compound investigated in this work, which superconducts at tempera-
|
| 56 |
+
tures ! ≤ !! = 20K.
|
| 57 |
+
|
| 58 |
+
Insulator
|
| 59 |
+
Superconductor
|
| 60 |
+
3
|
| 61 |
+
sensitive terahertz time-domain spectroscopy. The transient optical properties displayed
|
| 62 |
+
in Fig. 2c are reminiscent of those of the equilibrium superconducting state measured in
|
| 63 |
+
the same material at T ≪ T! = 20 K (cf. Fig. 2b), and are suggestive of transient high
|
| 64 |
+
temperature superconductivity. These signatures consist of a saturated reflectivity, a gap
|
| 65 |
+
in the real part of the optical conductivity +"(-), and an imaginary conductivity +#(-)
|
| 66 |
+
which diverges towards low frequencies as ~1/-. The divergent +#(-) implies (through
|
| 67 |
+
Kramers-Kronig relations) the presence of a peak in +" centred at zero frequency, with a
|
| 68 |
+
width limited by the lifetime of the state which also determines the carrier mobility.
|
| 69 |
+
These data were obtained by accounting for the inhomogeneous excitation of the probed
|
| 70 |
+
volume using a multilayer model. Here we show the results of this reconstruction under
|
| 71 |
+
the assumption of a linear (open symbols) and sublinear (filled symbols)20 dependence of
|
| 72 |
+
the photo-induced changes in the terahertz refractive index on the mid-infrared pump
|
| 73 |
+
fluence, as detailed in supplementary section S6. Allowing for a finite temperature super-
|
| 74 |
+
conductor, in which a varying density of uncondensed quasi-particles also contributes to
|
| 75 |
+
the terahertz response, the superconducting-like nature of the transient state is inde-
|
| 76 |
+
pendent of the specific choice of assumption. Only quantitative differences, associated
|
| 77 |
+
with the relative densities of induced superfluid and heated quasi-particles, which can be
|
| 78 |
+
extracted by fitting with a two-fluid model, emerge.
|
| 79 |
+
Note that the enhancement of conductivity observed in these experiments is not con-
|
| 80 |
+
nected to an increase in the carrier density, but is solely caused by a transfer of spectral
|
| 81 |
+
weight from the real part (resistive) to the imaginary part (inductive) of the conductivity,
|
| 82 |
+
and hence reflects a colossal increase in the carrier mobility at constant density.
|
| 83 |
+
Three spectrally-integrated figures of merit are extracted from the snapshots of R(-, 2),
|
| 84 |
+
+"(-, 2) and +#(-, 2), and plotted as a function of pump-probe time delay 2 in Fig. 2e,
|
| 85 |
+
showing the time evolution of the system.
|
| 86 |
+
|
| 87 |
+
|
| 88 |
+
4
|
| 89 |
+
|
| 90 |
+
Figure 2: Photo-induced metastable superconductivity in K3C60 generated with intense 170
|
| 91 |
+
meV excitation pulses. (a) Schematic of the experimental set-up. Pump pulses with 170 meV pho-
|
| 92 |
+
ton energy were generated in an optical parametric amplifier (OPA) and subsequent difference fre-
|
| 93 |
+
quency generation (DFG) of the signal and idler beams. These pulses were stretched to a duration
|
| 94 |
+
of ~1 ps by linear propagation in a highly dispersive CaF2 rod. The photoinduced changes in the far-
|
| 95 |
+
infrared optical properties of K3C60 were detected with phase-sensitive transient THz time-domain
|
| 96 |
+
spectroscopy. (b) Reflectivity (sample–diamond interface), real and imaginary part of the optical
|
| 97 |
+
conductivity of K3C60 measured upon cooling across the equilibrium superconducting transition.
|
| 98 |
+
The blue shading indicates the change of spectral weight in these quantities across the thermally
|
| 99 |
+
driven superconducting transition. (c) Same quantities measured at equilibrium (red lines) and
|
| 100 |
+
10 ps after excitation (filled and open symbols). The data in filled (open) symbols are obtained ac-
|
| 101 |
+
counting for the inhomogeneous excitation of the probed volume under the assumption of a square
|
| 102 |
+
root (linear) fluence dependence of the photo-induced changes in the complex refractive index of
|
| 103 |
+
the material (Supplementary Section S6). The blue shading indicates the change of spectral weight
|
| 104 |
+
in these quantities after photo-excitation. The blue solid lines are fits to the transient optical data
|
| 105 |
+
with a Drude-Lorentz model (Supplementary Section S7). These data were acquired at a base tem-
|
| 106 |
+
perature T = 100 K with an excitation fluence of 18 mJ cm-2. (d) Same quantities as in (c) but meas-
|
| 107 |
+
ured at a base temperature T = 295 K with an excitation fluence of 18 mJ cm-2. (e) Time dependence
|
| 108 |
+
of the average reflectivity, average real part of the optical conductivity &"((), and light-induced “su-
|
| 109 |
+
perfluid density” extracted from a two-fluid model fit and expressed as a fraction of the total charge
|
| 110 |
+
carrier density. All quantities are evaluated in the region of the photo-induced gap (5–10 meV).
|
| 111 |
+
Filled and open symbols indicate the results of two different reconstructions as in (c). The red dotted
|
| 112 |
+
lines indicate the value of the corresponding quantity at equilibrium. These data were acquired at a
|
| 113 |
+
base temperature T = 100 K with a fluence of 18 mJ cm−2 and a pump-pulse duration of ~1 ps.
|
| 114 |
+
|
| 115 |
+
a
|
| 116 |
+
3-Stage OPA
|
| 117 |
+
WLG
|
| 118 |
+
DFG
|
| 119 |
+
Ti:SaOscillator
|
| 120 |
+
Ti:SaAmplifierx2
|
| 121 |
+
THz gen.
|
| 122 |
+
b
|
| 123 |
+
d
|
| 124 |
+
e
|
| 125 |
+
1.0
|
| 126 |
+
Reflectivity*
|
| 127 |
+
Reflectivity
|
| 128 |
+
1.0
|
| 129 |
+
0.5
|
| 130 |
+
0.5
|
| 131 |
+
25K > Tc
|
| 132 |
+
Equilibrium
|
| 133 |
+
Equilibrium
|
| 134 |
+
18 mJ cm-2
|
| 135 |
+
5K< Tc
|
| 136 |
+
Photoexcited
|
| 137 |
+
Photoexcited
|
| 138 |
+
0.0
|
| 139 |
+
0.0
|
| 140 |
+
900
|
| 141 |
+
Equil.
|
| 142 |
+
T = 100 K
|
| 143 |
+
T = 295 K
|
| 144 |
+
T= i0 ps
|
| 145 |
+
= iops
|
| 146 |
+
cm
|
| 147 |
+
0%
|
| 148 |
+
Gapping
|
| 149 |
+
cm
|
| 150 |
+
600
|
| 151 |
+
150
|
| 152 |
+
300
|
| 153 |
+
*
|
| 154 |
+
6
|
| 155 |
+
6
|
| 156 |
+
100%
|
| 157 |
+
0
|
| 158 |
+
900
|
| 159 |
+
1.0
|
| 160 |
+
cm
|
| 161 |
+
600
|
| 162 |
+
0.5
|
| 163 |
+
300
|
| 164 |
+
(S
|
| 165 |
+
02
|
| 166 |
+
102040
|
| 167 |
+
102040
|
| 168 |
+
04
|
| 169 |
+
102040
|
| 170 |
+
C
|
| 171 |
+
0 5 10
|
| 172 |
+
50
|
| 173 |
+
100
|
| 174 |
+
Energy (meV) Energy (meV) Energy (meV)
|
| 175 |
+
Time (ps)
|
| 176 |
+
5
|
| 177 |
+
The first two quantities are the frequency-averaged values of the reflectivity and of +"(-)
|
| 178 |
+
below the energy gap, for which a zero-temperature superconductor with infinite lifetime
|
| 179 |
+
would give values of 1 and 0 respectively. The third figure of merit is the fractional super-
|
| 180 |
+
fluid density which is proportional
|
| 181 |
+
to the divergence of +#(-). This is determined by fitting the photoexcited optical proper-
|
| 182 |
+
ties with a two-fluid model where one fluid represents the remaining normal carriers with
|
| 183 |
+
a finite scattering rate and the other has zero scattering rate, giving a superconducting-
|
| 184 |
+
like contribution. Details of this fitting procedure are given in supplementary section S7.
|
| 185 |
+
For low excitation fluences the system becomes superconducting-like after photoexcita-
|
| 186 |
+
tion, and relaxes on a time scale of a few picoseconds. As already seen in the spectrally
|
| 187 |
+
resolved measurements, for high excitation fluences the system enters a metastable re-
|
| 188 |
+
gime in which the superconducting-like optical properties persist for much longer times,
|
| 189 |
+
up to several nanoseconds.
|
| 190 |
+
We note that the temperature dependence reported in Ref. 12 shows transient supercon-
|
| 191 |
+
ducting-like optical properties up to a temperature of 150-200 K. For higher tempera-
|
| 192 |
+
tures the gapping and extracted superfluid density are severely reduced. Examples of such
|
| 193 |
+
spectra measured at room temperature are shown in Fig. 2d. Nevertheless, the pressure
|
| 194 |
+
scaling reported in Ref. 13 suggests that traces of non-equilibrium superconductivity may
|
| 195 |
+
survive up to higher temperatures, raising the prospect that with more effective driving a
|
| 196 |
+
full manifestation of the metastable superconducting-like state may be possible at 300 K.
|
| 197 |
+
To date, these experiments have been limited to excitation photon energies between 80
|
| 198 |
+
and 165 meV (20-40 THz), such that a more comprehensive search for a dominant excita-
|
| 199 |
+
tion frequency scale has remained out of reach. Many potentially important resonances at
|
| 200 |
+
lower frequencies (ℎ4 < 80 meV) have remained unexplored, primarily due to the lack of
|
| 201 |
+
a suitable high-intensity pump source that operates in this range. In the present work, we
|
| 202 |
+
explore excitation at energies between 24 and 80 meV (6-20 THz).
|
| 203 |
+
|
| 204 |
+
|
| 205 |
+
6
|
| 206 |
+
|
| 207 |
+
Figure 3: Photo-induced metastable superconductivity in K3C60 generated with 41 meV exci-
|
| 208 |
+
tation pulses. (a) Schematic of the experimental set-up. Pump pulses with 41 meV (10 THz) photon
|
| 209 |
+
energy are generated in a twin optical parametric amplifier (OPA) and subsequent chirped-pulse
|
| 210 |
+
difference frequency generation (DFG) of the two stretched signal beams. The photoinduced
|
| 211 |
+
changes in the far-infrared optical properties of K3C60 are detected with phase-sensitive transient
|
| 212 |
+
THz time-domain spectroscopy. (b) Reflectivity (sample–diamond interface), real and imaginary
|
| 213 |
+
part of the optical conductivity of K3C60 measured at equilibrium (red lines) and 50 ps after excita-
|
| 214 |
+
tion (filled and open symbols). The data in filled (open) symbols are obtained accounting for the
|
| 215 |
+
inhomogeneous excitation of the probed volume under the assumption of a square root (linear) flu-
|
| 216 |
+
ence dependence of the photo-induced changes in the complex refractive index of the material. The
|
| 217 |
+
blue shading indicates the change of spectral weight in these quantities after photo-excitation. These
|
| 218 |
+
data were acquired at a base temperature T = 100 K with pump pulses tuned to 41 meV (10 THz)
|
| 219 |
+
center frequency and excitation fluence of 0.4 mJ cm-2. (c) Same quantities as in (b) but measured
|
| 220 |
+
10 ps after photoexcitation at a base temperature T = 295 K. (d) Same quantities as in (c) but meas-
|
| 221 |
+
ured 50 ps after photoexcitation. (e) Time dependence of the average reflectivity, average real part
|
| 222 |
+
of the optical conductivity &"((), and light-induced “superfluid density” extracted from a two-fluid
|
| 223 |
+
model fit and expressed as a fraction of the total charge carrier density. All quantities are evaluated
|
| 224 |
+
in the region of the photo-induced gap (5–10 meV). Filled and open symbols indicate the results of
|
| 225 |
+
two different reconstruction as in (b). The inset in the top panel highlights the early time delays
|
| 226 |
+
region where light amplification (* > 1) is observed (red shading). The red dotted lines indicate the
|
| 227 |
+
value of the corresponding quantity at equilibrium. These data were acquired at a base temperature
|
| 228 |
+
T = 100 K with pump pulses tuned to 45 meV (11 THz) photon energy and excitation fluence of
|
| 229 |
+
0.5 mJ cm-2
|
| 230 |
+
|
| 231 |
+
a
|
| 232 |
+
2x3-stageOPAs
|
| 233 |
+
Pulsestretchers
|
| 234 |
+
WLG
|
| 235 |
+
DFG
|
| 236 |
+
THz gen.
|
| 237 |
+
Ti:SaAmplifier
|
| 238 |
+
b
|
| 239 |
+
e
|
| 240 |
+
Reflectivity
|
| 241 |
+
Reflectivity*
|
| 242 |
+
.0
|
| 243 |
+
0.5
|
| 244 |
+
0.5
|
| 245 |
+
Equilibrium
|
| 246 |
+
Equilibrium
|
| 247 |
+
Equilibrium
|
| 248 |
+
Photoexcited
|
| 249 |
+
Photoexcited
|
| 250 |
+
Photoexcited
|
| 251 |
+
0.0
|
| 252 |
+
0.0
|
| 253 |
+
900
|
| 254 |
+
T=100K
|
| 255 |
+
T= 295K
|
| 256 |
+
T= 295K
|
| 257 |
+
0%
|
| 258 |
+
cm
|
| 259 |
+
T = 50 ps
|
| 260 |
+
T = 10 ps
|
| 261 |
+
T = 50 ps
|
| 262 |
+
600
|
| 263 |
+
cm
|
| 264 |
+
Gapping
|
| 265 |
+
150
|
| 266 |
+
0.5 mJ cm-2
|
| 267 |
+
300
|
| 268 |
+
*
|
| 269 |
+
100%
|
| 270 |
+
0
|
| 271 |
+
6
|
| 272 |
+
900
|
| 273 |
+
1.0
|
| 274 |
+
600
|
| 275 |
+
ntot
|
| 276 |
+
0.5
|
| 277 |
+
nsf
|
| 278 |
+
300
|
| 279 |
+
6
|
| 280 |
+
0
|
| 281 |
+
4
|
| 282 |
+
102040
|
| 283 |
+
4102040
|
| 284 |
+
41020
|
| 285 |
+
0 5 10
|
| 286 |
+
50
|
| 287 |
+
100
|
| 288 |
+
Energy (meV)
|
| 289 |
+
Energy (meV)
|
| 290 |
+
E
|
| 291 |
+
Energy (meV)
|
| 292 |
+
Time (ps)
|
| 293 |
+
7
|
| 294 |
+
This energy range hosts a number of excitations, both vibrational (phonons) and elec-
|
| 295 |
+
tronic in nature, including a broad polaronic peak seen in +" centered at approximately
|
| 296 |
+
60 meV (15 THz). The possible relevance of this excitation has been highlighted in Ref. 21,
|
| 297 |
+
although this prediction could not be tested to date.
|
| 298 |
+
To achieve wide tuneability, we made use of a terahertz source based on chirped pulse
|
| 299 |
+
difference frequency generation, mixing the near-infrared signal beams of two phase-
|
| 300 |
+
locked optical parametric amplifiers22. This source, illustrated schematically in Fig. 3a and
|
| 301 |
+
described in detail in supplementary section S4, was used to generate narrow-bandwidth
|
| 302 |
+
pulses with photon energies spanning the range from 24 to 145 meV (6-35 THz). All meas-
|
| 303 |
+
urements reported here were carried out with an excitation bandwidth of ~4 meV
|
| 304 |
+
(1 THz) and ~600 fs pulse duration. The same probing protocol as that reported in Fig. 2
|
| 305 |
+
was utilized here to detect changes in the complex optical properties for probe energies
|
| 306 |
+
spanning 4-18 meV (1-4.5 THz).
|
| 307 |
+
Figures 3b-d show reflectivity and complex conductivity spectra measured after photoex-
|
| 308 |
+
citation with pulses tuned to 41 meV photon energy (l ~ 30 µm, ) ~ 10 THz) at base tem-
|
| 309 |
+
peratures of 100 K and room temperature, respectively. Figure 3e displays the time-evo-
|
| 310 |
+
lution of the optical properties. The response is very similar to the case reported in Fig. 2
|
| 311 |
+
for 170 meV (41 THz) excitation, manifested on metastable timescales but persisting here
|
| 312 |
+
up to room temperature – despite an almost two orders of magnitude weaker excitation
|
| 313 |
+
fluence.
|
| 314 |
+
Figure 4a shows the scaling with fluence of the below-gap averaged values of 8(-) and
|
| 315 |
+
+"(-), as well as the fractional superfluid density in response to photoexcitation at
|
| 316 |
+
170 meV (41 THz) and 41 meV (10 THz). These measurements were carried out at a
|
| 317 |
+
pump-probe time delay of 10 ps, and thus refer to the metastable phase. The figure shows
|
| 318 |
+
how all figures of merit approach their equilibrium superconducting-state values as the
|
| 319 |
+
|
| 320 |
+
|
| 321 |
+
8
|
| 322 |
+
fluence increases, with the fluence required being approximately 50 times less for 41 meV
|
| 323 |
+
(10 THz) compared to 170 meV (41 THz) excitation.
|
| 324 |
+
Similar fluence dependence measurements were carried out by varying the photon en-
|
| 325 |
+
ergy of the pump and maintaining a constant 4 meV (1 THz) bandwidth with 600 fs pulse
|
| 326 |
+
duration. For all excitation photon energies between 24 meV (6 THz) and 145 meV
|
| 327 |
+
(35 THz) the photoinduced changes in the optical properties were qualitatively similar to
|
| 328 |
+
those shown in Figs. 2, 3 with only the size of the response for a given fluence differing.
|
| 329 |
+
From each fluence dependence we extracted a figure of merit for the photo-susceptibility,
|
| 330 |
+
|
| 331 |
+
Figure 4: Scaling of the out-of-equilibrium features of photo-induced metastable supercon-
|
| 332 |
+
ductivity in K3C60. (a) Fluence dependence of the average reflectivity, average real part of the op-
|
| 333 |
+
tical conductivity &"((), and light-induced “superfluid density” extracted from a two-fluid model fit
|
| 334 |
+
and expressed as a fraction of the total charge carrier density. All quantities are evaluated in the
|
| 335 |
+
region of the photo-induced gap (5–10 meV). Red and blue symbols indicate measurements with
|
| 336 |
+
excitation pulses tuned to 41 meV (10 THz) and 170 meV (41 THz) central frequency. The red dotted
|
| 337 |
+
lines indicate the value of the corresponding quantity at equilibrium. These data were acquired at a
|
| 338 |
+
base temperature T = 100 K, at a time-delay ∆t = 10ps, and with a pump pulse duration of ~600 fs.
|
| 339 |
+
(b) Frequency dependence of the photo-susceptibility of K3C60 defined as the gradient of the lost
|
| 340 |
+
spectral weight in &" in the low-fluence limit (Supplementary Section S8) measured 10 ps and 50 ps
|
| 341 |
+
after photo-excitation. These measurements were carried out at a base temperature T = 100 K.
|
| 342 |
+
These data are obtained by accounting for the inhomogeneous excitation of the probed volume un-
|
| 343 |
+
der the assumption of a square root fluence dependence of the photo-induced changes in the com-
|
| 344 |
+
plex refractive index of the material.
|
| 345 |
+
|
| 346 |
+
41 me
|
| 347 |
+
170 meV
|
| 348 |
+
9
|
| 349 |
+
defined as the rate of growth of the +" gap with excitation fluence in the limit of low flu-
|
| 350 |
+
ence (see supplementary section S8). Plots of the pump-frequency-dependent photo-sus-
|
| 351 |
+
ceptibility are shown in Fig. 4b for both 10 ps and 50 ps pump-probe time delay. A peak
|
| 352 |
+
centered at 41 meV (10 THz) with approximately 16 meV FWHM bandwidth is observed
|
| 353 |
+
in these measurements. In the next section we will discuss three distinct energy scales
|
| 354 |
+
which coincide with this resonance, sequentially these relate to “on-ball” orbital excita-
|
| 355 |
+
tions, phonons and finally excitons.
|
| 356 |
+
Superconductivity in alkali-doped fullerides is believed to be mediated by a dynamical
|
| 357 |
+
Jahn-Teller distortion, which leads to an effective negative Hund’s coupling for the orbit-
|
| 358 |
+
als of a single buckyball23 and to a low spin S=1/2 state. A theoretical model based on this
|
| 359 |
+
assumption has been successful at providing a quantitatively correct phase diagram for
|
| 360 |
+
fulleride superconductors, based on ab-initio calculations24,25. Within this model, the local
|
| 361 |
+
ground state of the system is a six-fold degenerate low-spin state, which features intra-
|
| 362 |
+
orbital pairs that de-localize over two molecular orbitals. As detailed in supplementary
|
| 363 |
+
section S10, a first set of local excited states also features such pairs, albeit with a different
|
| 364 |
+
angular momentum (i.e. a different inter-orbital phase for the delocalized pair). Ab-initio
|
| 365 |
+
calculations predict an energy splitting of 37 meV between these two sets of states24,25.
|
| 366 |
+
The observed resonance may therefore be related to the creation of interorbital pairs with
|
| 367 |
+
local angular momentum, which may also contribute to superconductivity, as suggested
|
| 368 |
+
in the Suhl-Kondo mechanism26,27. However, it is not yet clear how exactly this excitation
|
| 369 |
+
is transformed in the presence of tunneling between neighboring C60 molecules, and why
|
| 370 |
+
the creation of such pairs may support metastable superconductivity at such high tem-
|
| 371 |
+
peratures. Furthermore, as the local parity of this excited state would be different from
|
| 372 |
+
that of the ground state, condensation in this configuration may give rise to a supercon-
|
| 373 |
+
ductor with different symmetry. This possibility, whilst tantalizing, remains speculative
|
| 374 |
+
and should be tested with more comprehensive ultrafast probing methods.
|
| 375 |
+
|
| 376 |
+
|
| 377 |
+
10
|
| 378 |
+
Turning to phonon excitations, we also note that the 41 meV resonance frequency identi-
|
| 379 |
+
fied here coincides with an infrared-active T1u phonon which predominantly consists of
|
| 380 |
+
intramolecular motion of the C atoms. While the atomic motions of the 170 meV molecular
|
| 381 |
+
mode discussed previously in Ref. 12 are directed along the tangential directions of the
|
| 382 |
+
C603- molecule, those of the 41 meV mode are predominantly along the radial directions
|
| 383 |
+
(see supplementary section S9). By performing frozen phonon calculations using density
|
| 384 |
+
functional theory (DFT) we evaluated the different impact of these distortions on the
|
| 385 |
+
three t1u molecular levels at the Fermi energy, which we map out from DFT wave functions
|
| 386 |
+
as maximally-localized Wannier functions (supplementary section S9). In the undistorted
|
| 387 |
+
C603- structure these molecular levels are degenerate. Applying a distortion along a T1u
|
| 388 |
+
coordinate lifts this degeneracy leaving a doubly degenerate t1u orbital lowered in energy.
|
| 389 |
+
This electronic configuration is prone to developing a Jahn-Teller distortion that may lead
|
| 390 |
+
to an enhanced negative Hund’s coupling, possibly facilitating the onset of superconduc-
|
| 391 |
+
tivity at higher temperatures.
|
| 392 |
+
The strength of the induced splitting is quadratic in the phonon coordinate and is more
|
| 393 |
+
significant for when driving the 41 meV mode compared to the 170 meV one, suggesting
|
| 394 |
+
that the observed resonance may arise from a more efficient manipulation of the elec-
|
| 395 |
+
tronic degrees of freedom when driving the 41 meV T1u mode.
|
| 396 |
+
Finally, we address the electronic excitations discussed in Ref. 21, in which the existence
|
| 397 |
+
of a polaronic mode was predicted at the same energy scales as the resonance reported
|
| 398 |
+
here. However, we also note that the proposed mechanism for the formation of the non-
|
| 399 |
+
equilibrium superconducting-like state was one in which the quasi-particles are cooled
|
| 400 |
+
incoherently via coupling to the polaronic bath. As already reported in Ref. 28 and shown
|
| 401 |
+
here in the inset to Fig. 3e, the response of the sample in the first few picoseconds after
|
| 402 |
+
photoexcitation yields amplification of the terahertz probe light, which is likely to reflect
|
| 403 |
+
coherent dynamics of the driven degrees of freedom. Assuming that the mechanism
|
| 404 |
+
|
| 405 |
+
|
| 406 |
+
11
|
| 407 |
+
proposed in Ref. 21 were to be valid, the early-time dynamics of that model would require
|
| 408 |
+
further investigation to understand how such coherences would arise at early times. The
|
| 409 |
+
amplification observed here and in Ref. 28 has so far been attributed to the existence of a
|
| 410 |
+
parametric resonance that couples amplitude (Higgs) modes to phase (Goldstone) modes,
|
| 411 |
+
an effect possible at the sample surface because of reduced screening.
|
| 412 |
+
We expect the significance of this discovery to be capitalized upon in future work. The
|
| 413 |
+
extreme efficiency improvement due to resonant enhancement, nearing two orders of
|
| 414 |
+
magnitude, is expected to also dramatically reduce unwanted dissipation. This, taken in
|
| 415 |
+
conjunction with the observed nanosecond-long lifetime suggests that excitation of the
|
| 416 |
+
sample with a train of pulses of only 400 µJ/cm2 delivered at 100 MHz repetition rate – as
|
| 417 |
+
determined by the inverse lifetime of this state - may yield continuous wave operation.
|
| 418 |
+
Because this effect is documented here to persist up to room temperature, continuous
|
| 419 |
+
wave operation would likely have important practical implications. To make this regime
|
| 420 |
+
experimentally accessible, single order-of-magnitude improvements in the efficiency of
|
| 421 |
+
the process, or in the light matter coupling strength, combined with suitable develop-
|
| 422 |
+
ments in high repetition rate THz sources would be required.
|
| 423 |
+
|
| 424 |
+
Acknowledgments
|
| 425 |
+
The research leading to these results received funding from the European Research Council under
|
| 426 |
+
the European Union’s Seventh Framework Programme (FP7/2007-2013)/ERC Grant Agreement
|
| 427 |
+
No. 319286 (QMAC). We acknowledge support from the Deutsche Forschungsgemeinschaft (DFG)
|
| 428 |
+
via the Cluster of Excellence ‘The Hamburg Centre for Ultrafast Imaging’ (EXC 1074 – project ID
|
| 429 |
+
194651731). We thank Michael Volkmann and Peter Licht for their technical assistance. We are
|
| 430 |
+
also grateful to Boris Fiedler and Birger Höhling for their support in the fabrication of the elec-
|
| 431 |
+
tronic devices used on the measurement setup, and to Jörg Harms for assistance with graphics.
|
| 432 |
+
|
| 433 |
+
|
| 434 |
+
|
| 435 |
+
|
| 436 |
+
12
|
| 437 |
+
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|
| 438 |
+
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|
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| 497 |
+
Wang, E. et al. Nonlinear transport in a photo-induced superconductor. arXiv:2301.06425,
|
| 498 |
+
(2023).
|
| 499 |
+
20
|
| 500 |
+
Dodge, J. S., Lopez, L. & Sahota, D. G. Photoinduced Superconductivity Reconsidered: The
|
| 501 |
+
Role of Photoconductivity Profile Distortion. arXiv:2210.01114, (2022).
|
| 502 |
+
21
|
| 503 |
+
Nava, A., Giannetti, C., Georges, A., Tosatti, E. & Fabrizio, M. Cooling quasiparticles in A3C60
|
| 504 |
+
fullerides by excitonic mid-infrared absorption. Nature Physics 14, 154-159, (2018).
|
| 505 |
+
22
|
| 506 |
+
Liu, B. et al. Generation of narrowband, high-intensity, carrier-envelope phase-stable
|
| 507 |
+
pulses tunable between 4 and 18 THz. Opt. Lett. 42, 129-131, (2017).
|
| 508 |
+
23
|
| 509 |
+
Capone, M., Fabrizio, M., Castellani, C. & Tosatti, E. Strongly Correlated Superconductivity.
|
| 510 |
+
Science 296, 2364-2366, (2002).
|
| 511 |
+
24
|
| 512 |
+
Nomura, Y., Sakai, S., Capone, M. & Arita, R. Unified understanding of superconductivity
|
| 513 |
+
and Mott transition in alkali-doped fullerides from first principles. Science Advances 1,
|
| 514 |
+
e1500568, (2015).
|
| 515 |
+
25
|
| 516 |
+
Nomura, Y., Sakai, S., Capone, M. & Arita, R. Exotics-wave superconductivity in alkali-doped
|
| 517 |
+
fullerides. Journal of Physics: Condensed Matter 28, 153001, (2016).
|
| 518 |
+
26
|
| 519 |
+
Suhl, H. Dispersion Theory of the Kondo Effect. Physical Review 138, A515-A523, (1965).
|
| 520 |
+
27
|
| 521 |
+
Kondo, J. Resistance Minimum in Dilute Magnetic Alloys. Progress of Theoretical Physics
|
| 522 |
+
32, 37-49, (1964).
|
| 523 |
+
28
|
| 524 |
+
Buzzi, M. et al. Higgs-Mediated Optical Amplification in a Nonequilibrium Superconductor.
|
| 525 |
+
Physical Review X 11, 011055, (2021).
|
| 526 |
+
|
| 527 |
+
|
| 528 |
+
|
| 529 |
+
|
| 530 |
+
14
|
| 531 |
+
Giant resonant enhancement for photo-induced
|
| 532 |
+
superconductivity in K3C60
|
| 533 |
+
E. Rowe1,*, B. Yuan1, M. Buzzi1, G. Jotzu1, Y. Zhu1, M. Fechner1, M. Först1, B. Liu1,2
|
| 534 |
+
D. Pontiroli3, M. Riccò3, A. Cavalleri1,4,*
|
| 535 |
+
|
| 536 |
+
1 Max Planck Institute for the Structure and Dynamics of Matter, Hamburg, Germany
|
| 537 |
+
2 Paul Scherrer Institute, Villigen, Switzerland
|
| 538 |
+
3 Dipartimento di Scienze Matematiche, Fisiche e Informatiche, Università degli Studi di Parma, Italy
|
| 539 |
+
4 Department of Physics, Clarendon Laboratory, University of Oxford, United Kingdom
|
| 540 |
+
* e-mail: edward.rowe@mpsd.mpg.de, andrea.cavalleri@mpsd.mpg.de
|
| 541 |
+
|
| 542 |
+
|
| 543 |
+
Supplemental Material
|
| 544 |
+
S1. Sample growth and characterization
|
| 545 |
+
S2. Determination of the equilibrium optical properties
|
| 546 |
+
S3. High fluence mid-infrared source
|
| 547 |
+
S4. Frequency-tunable narrowband terahertz and mid-infrared source
|
| 548 |
+
S5. Measurements of the transient THz reflectivity
|
| 549 |
+
S6. Determination of the transient optical properties
|
| 550 |
+
S7. Fitting the transient optical spectra
|
| 551 |
+
S8. Extracting the frequency-dependent photosusceptibility
|
| 552 |
+
S9. Density functional theory calculations
|
| 553 |
+
S10. Local electronic hamiltonian calculations
|
| 554 |
+
|
| 555 |
+
|
| 556 |
+
|
| 557 |
+
|
| 558 |
+
|
| 559 |
+
|
| 560 |
+
|
| 561 |
+
15
|
| 562 |
+
S1. Sample growth and characterization
|
| 563 |
+
|
| 564 |
+
The K3C60 powder pellets used in this work were prepared and characterized as reported
|
| 565 |
+
previously1-3. Stoichiometric amounts of ground C60 powder and potassium were placed
|
| 566 |
+
in a sealed pyrex vial, which was evacuated to a pressure of 10-6 mbar. Whilst keeping the
|
| 567 |
+
C60 powder and solid potassium separated, the vial was kept at 523 K for 72 h and then
|
| 568 |
+
at 623 K for 28 h such that the C60 powder was exposed to pure potassium vapor. The vial
|
| 569 |
+
was then opened inside an Ar glovebox (<0.1 ppm O2 and H2O), where the powder was
|
| 570 |
+
reground and pelletized before annealing at 623K for 5 days. X-ray diffraction
|
| 571 |
+
measurements were then carried out on the resulting K3C60 powder, which confirmed
|
| 572 |
+
that it was phase pure, with an average grain size ranging between 100 and 400 nm. The
|
| 573 |
+
static superconducting transition temperature was measured to be 19.8 K (in agreement
|
| 574 |
+
with literature values) via magnetic susceptibility measurements upon zero field cooling
|
| 575 |
+
and cooling in field with a field strength of 400 A/m.
|
| 576 |
+
|
| 577 |
+
|
| 578 |
+
|
| 579 |
+
Figure S1.1: a. X-ray diffraction data and single f.c.c. phase Rietveld refinement for the K3C60
|
| 580 |
+
powder used in this work. b. Temperature dependence of the sample magnetic susceptibility
|
| 581 |
+
measured by SQUID magnetometry upon cooling without (ZFC: zero field cooling) and with a
|
| 582 |
+
magnetic field applied (FCC: field cooled cooling).
|
| 583 |
+
|
| 584 |
+
|
| 585 |
+
|
| 586 |
+
observed
|
| 587 |
+
(10emu/(g0e)
|
| 588 |
+
calculated
|
| 589 |
+
residual
|
| 590 |
+
reflections
|
| 591 |
+
20
|
| 592 |
+
ZFC
|
| 593 |
+
FCC
|
| 594 |
+
30
|
| 595 |
+
40
|
| 596 |
+
50
|
| 597 |
+
10
|
| 598 |
+
20
|
| 599 |
+
30
|
| 600 |
+
40
|
| 601 |
+
50
|
| 602 |
+
60
|
| 603 |
+
5
|
| 604 |
+
10
|
| 605 |
+
15
|
| 606 |
+
20
|
| 607 |
+
2A
|
| 608 |
+
tdearees
|
| 609 |
+
Temperature
|
| 610 |
+
|
| 611 |
+
16
|
| 612 |
+
S2. Determination of the equilibrium optical properties
|
| 613 |
+
|
| 614 |
+
The equilibrium reflectivity was measured for photon energies between 5 meV and 500
|
| 615 |
+
meV using a commercial Fourier-transform infrared spectrometer (FTIR) equipped with
|
| 616 |
+
a microscope at the SISSI beamline in the Elettra Synchrotron Facility (Trieste, Italy), as
|
| 617 |
+
reported previously1-3. The sample was pressed by a diamond window into a sealed
|
| 618 |
+
holder in order to obtain an optically flat interface and prevent exposure to air. This
|
| 619 |
+
procedure was carried out inside an Ar filled glove box (<0.1 ppm O2 and H2O) before the
|
| 620 |
+
sealed sample was removed and mounted on a He cooled cryostat to enable temperature
|
| 621 |
+
dependent measurements. The K3C60 reflectivity spectra were referenced against a gold
|
| 622 |
+
mirror placed at the sample position.
|
| 623 |
+
In order to extract the complex optical conductivity a Kramers-Kronig algorithm for
|
| 624 |
+
samples in contact with a transparent window4 was used. This requires data at all
|
| 625 |
+
frequencies, which were obtained, at low energies (<5 meV) using an extrapolation based
|
| 626 |
+
on a Drude-Lorentz fit, and at high energies (>500 meV) using data measured on single
|
| 627 |
+
crystal samples reported in Refs. 5,6.
|
| 628 |
+
The equilibrium properties are shown in figure S2.1 for temperatures of 100 K and 300
|
| 629 |
+
K. This and further data measured at different temperatures and pressures were already
|
| 630 |
+
reported in Refs. 1,2 and discussed also in comparison with data obtained from single
|
| 631 |
+
crystals.
|
| 632 |
+
These data were fitted with a Drude-Lorentz model, which is given by the following
|
| 633 |
+
equation:
|
| 634 |
+
𝜎!(𝜔) + 𝑖𝜎"(𝜔) = 𝜔#"
|
| 635 |
+
4𝜋
|
| 636 |
+
1
|
| 637 |
+
𝛾$ − 𝑖𝜔 + 𝜔#,&'(
|
| 638 |
+
"
|
| 639 |
+
4𝜋
|
| 640 |
+
𝜔
|
| 641 |
+
𝑖.𝜔),&'(
|
| 642 |
+
"
|
| 643 |
+
− 𝜔"/ + 𝛾&'(𝜔
|
| 644 |
+
Here the first term represents the Drude response of the free carriers with 𝜔# and 𝛾$
|
| 645 |
+
representing the plasma frequency and scattering rate respectively, whereas the second
|
| 646 |
+
term captures the mid infrared absorption in the form of a Lorentz oscillator centered at
|
| 647 |
+
frequency 𝜔),&'( with plasma frequency 𝜔#,&'( and damping rate 𝛾&'(. The equilibrium
|
| 648 |
+
data reported here was used to normalize the transient optical spectra of K3C60 measured
|
| 649 |
+
upon photoexcitation, as discussed in detail in section S6.
|
| 650 |
+
|
| 651 |
+
|
| 652 |
+
|
| 653 |
+
|
| 654 |
+
|
| 655 |
+
17
|
| 656 |
+
Figure S2.1: Equilibrium optical properties (reflectivity, real, and imaginary part of the optical
|
| 657 |
+
conductivity) of K3C60 measured at a temperature of 100 K (blue) and 300 K (green). The black
|
| 658 |
+
dashed curve is a Drude-Lorentz fit to the optical conductivity at 100 K in the range from 3 meV
|
| 659 |
+
to 60 meV as described in the text.
|
| 660 |
+
|
| 661 |
+
S3. High fluence mid-infrared source
|
| 662 |
+
|
| 663 |
+
For the data reported in figure 2 and in figure 4(a) at 170 meV (41 THz) excitation, the
|
| 664 |
+
pump pulses were generated via difference frequency mixing (DFG) of the signal and idler
|
| 665 |
+
output of a three-stage home-built optical parametric amplifier (OPA). A commercial
|
| 666 |
+
Ti:Al2O3 amplifier delivering 60 fs duration pulses at 800 nm central wavelength was used
|
| 667 |
+
to drive the OPA, and the DFG process was performed using a 0.5 mm thick GaSe crystal,
|
| 668 |
+
resulting in ~100 fs long pulses. The 170 meV pulses were then propagated through a
|
| 669 |
+
highly dispersive 16 mm long CaF2 rod, stretching their duration to ~1 ps. The spectrum
|
| 670 |
+
of the pump pulses was characterized using a home built FTIR spectrometer. Their
|
| 671 |
+
duration was measured by cross-correlation with a synchronized, 35 fs long, 800 nm
|
| 672 |
+
wavelength pulse in a 50 μm thick GaSe crystal. While a certain degree of tunability is also
|
| 673 |
+
given by this source, its useful operation range spans between 80 and 320 meV, hence it
|
| 674 |
+
was only used for the high-intensity experiments at 170 meV excitation.
|
| 675 |
+
|
| 676 |
+
|
| 677 |
+
|
| 678 |
+
|
| 679 |
+
|
| 680 |
+
900
|
| 681 |
+
E
|
| 682 |
+
900㎡
|
| 683 |
+
1.0
|
| 684 |
+
300 K
|
| 685 |
+
100K
|
| 686 |
+
Reflectivity
|
| 687 |
+
T-
|
| 688 |
+
T-
|
| 689 |
+
600
|
| 690 |
+
600
|
| 691 |
+
Fit 100 K
|
| 692 |
+
0.5
|
| 693 |
+
300
|
| 694 |
+
300
|
| 695 |
+
02
|
| 696 |
+
0.04
|
| 697 |
+
0
|
| 698 |
+
10
|
| 699 |
+
30
|
| 700 |
+
100
|
| 701 |
+
410
|
| 702 |
+
30
|
| 703 |
+
100
|
| 704 |
+
4
|
| 705 |
+
10
|
| 706 |
+
30
|
| 707 |
+
100
|
| 708 |
+
Energy (meV)
|
| 709 |
+
Energy (meV)
|
| 710 |
+
Energy (meV)
|
| 711 |
+
|
| 712 |
+
18
|
| 713 |
+
S4. Frequency-tunable narrowband terahertz and mid-infrared source
|
| 714 |
+
|
| 715 |
+
For the experiments that required tunability of the excitation pulses down to the THz gap,
|
| 716 |
+
a different source was used. This source is based on the principle of chirped-pulse
|
| 717 |
+
difference frequency generation (CP-DFG) in organic non-linear optical crystals, namely
|
| 718 |
+
DAST and DSTMS of approximately 600 μm thickness. The principle of operation of this
|
| 719 |
+
new source is described in detail in Ref. 7. A commercial Ti:Al2O3 amplifier is used to drive
|
| 720 |
+
two identical three-stage OPAs which are seeded by the same white-light, such that the
|
| 721 |
+
signal beams have the same phase-fluctuations. The ~100 fs signal pulses are then
|
| 722 |
+
chirped using a pair of transmission-grating-based stretchers as depicted in figure 3(a).
|
| 723 |
+
This arrangement enables continuous tuning of the pulse durations by varying the
|
| 724 |
+
distance between the gratings in each pair, effectively enabling continuous tuning of the
|
| 725 |
+
pump-pulse bandwidth. For this experiment the pump pulse bandwidth was kept
|
| 726 |
+
constant at 4 meV by maintaining a signal pulse duration of ~600 fs, as measured using a
|
| 727 |
+
home-built second harmonic-based Frequency-Resolved-Optical-Gating (FROG) device.
|
| 728 |
+
Frequency tuning of the generated excitation pulses was carried out both by varying the
|
| 729 |
+
central wavelengths of the two OPA signal beams, and by varying the time delay between
|
| 730 |
+
the chirped signal pulses in the DFG crystal (for fine tuning). For each measurement the
|
| 731 |
+
pump frequency spectrum was measured via FTIR (Fourier Transform Infrared
|
| 732 |
+
Spectroscopy).
|
| 733 |
+
|
| 734 |
+
S5. Measurements of the transient THz reflectivity
|
| 735 |
+
|
| 736 |
+
The experiments presented in Figures 2, 3, and 4 were performed on compacted K3C60
|
| 737 |
+
powder pellets pressed against a diamond window to ensure an optically flat interface.
|
| 738 |
+
As K3C60 is water and oxygen sensitive, the pellets were sealed in an air-tight holder and
|
| 739 |
+
all sample handling operations were performed in an Argon filled glove box with <0.1
|
| 740 |
+
ppm O2 and H2O. The sample holder was then installed at the end of a commercial Helium
|
| 741 |
+
cold-finger (base temperature 5K), to cool the pellets down to a temperature of 100 K.
|
| 742 |
+
The changes in the properties of the sample following photoexcitation were measured
|
| 743 |
+
using time-domain THz-spectroscopy.
|
| 744 |
+
|
| 745 |
+
|
| 746 |
+
|
| 747 |
+
19
|
| 748 |
+
The mid-infrared pump induced changes in the low frequency optical properties, were
|
| 749 |
+
retrieved using transient THz time domain spectroscopy in two different experimental
|
| 750 |
+
setups. The THz probe pulses were generated via optical rectification in a 0.2 mm thick
|
| 751 |
+
(110)-cut GaP crystal starting from 800 nm pulses with a duration of ~80 fs and 35 fs,
|
| 752 |
+
respectively. Whilst in one setup these 800 nm were derived from the same laser used
|
| 753 |
+
for pumping the source described in section S4, the 35 fs, 800 nm pulses were generated
|
| 754 |
+
by a second Ti:Al2O3 amplifier optically synchronized to that used to pump the high-
|
| 755 |
+
intensity mid-infrared source described in section S3. The THz probe pulses were then
|
| 756 |
+
focused onto the sample with incidence angles of 30 and 0 degrees, respectively. After
|
| 757 |
+
reflection from the sample, the electric field profile of the THz pulses was reconstructed
|
| 758 |
+
in a standard electro-optic sampling setup, using a (110)-cut 0.2 mm GaP crystal
|
| 759 |
+
supported on a 1 mm thick (100)-cut GaP substrate to delay internal reflections. The
|
| 760 |
+
setup combined with the frequency tunable narrowband source had a measurement
|
| 761 |
+
bandwidth that extended between 4 and 18 meV, while the other spanned between
|
| 762 |
+
4 meV to 29 meV. The time resolution of both setups is determined by the measurement
|
| 763 |
+
bandwidth and is ~250 fs and ~150 fs respectively.
|
| 764 |
+
To minimize the effects on the pump-probe time resolution due to the finite duration of
|
| 765 |
+
the THz probe pulse, the experiments were performed as described in Refs. 8, 9. The
|
| 766 |
+
pump-probe time delay was controlled by fixing the delay between the 800 nm gating
|
| 767 |
+
pulse and the mid-infrared pump pulse 𝜏. The transient THz field was then obtained by
|
| 768 |
+
scanning the delay 𝑡 relative to both.
|
| 769 |
+
In order to simultaneously retrieve both the ‘pump on’ (𝐸*+,
|
| 770 |
+
&- (𝑡, 𝜏)) and ‘pump off’
|
| 771 |
+
(𝐸*+,
|
| 772 |
+
&..(𝑡)) probe fields, a differential chopping scheme was deployed. The scheme was
|
| 773 |
+
different for the two above mentioned setup. For the narrowband, frequency tunable
|
| 774 |
+
setup which operated at a repetition rate of 1 kHz, the THz probe pulse was chopped at a
|
| 775 |
+
frequency of 500 Hz and the mid-infrared pump pulse was chopped at ~ 357 Hz. The
|
| 776 |
+
electro-optic sampling signal was then fed to two lock-in amplifiers reading out 𝑉/01! at
|
| 777 |
+
500 Hz and 𝑉/01" at 143 Hz respectively. For the high-intensity setup, operating at 2 kHz
|
| 778 |
+
repetition rate, the THz probe pulse was chopped at a frequency of 1 kHz and the mid-
|
| 779 |
+
infrared pump was chopped at 500 Hz. In this case, the electro-optic sampling signal was
|
| 780 |
+
filtered by two lock-in amplifiers operating at 1 kHz and 500 Hz respectively. 𝐸*+,
|
| 781 |
+
&..(𝑡) and
|
| 782 |
+
Δ𝐸*+,(𝑡, 𝜏) were then extracted from the signals in the two lock-ins using the following
|
| 783 |
+
formulas:
|
| 784 |
+
|
| 785 |
+
|
| 786 |
+
|
| 787 |
+
20
|
| 788 |
+
𝐸*+,
|
| 789 |
+
&..(𝑡) = 𝑉𝐿𝐼𝐴1(𝑡, 𝜏) − 𝛼𝑉𝐿𝐼𝐴2(𝑡, 𝜏)
|
| 790 |
+
Δ𝐸*+,(𝑡, 𝜏) = 𝐸*+,
|
| 791 |
+
&- (𝑡, 𝜏) − 𝐸*+,
|
| 792 |
+
&..(𝑡) = 𝛼𝑉𝐿𝐼𝐴2(𝑡, 𝜏)
|
| 793 |
+
|
| 794 |
+
where 𝛼 is a calibration constant determined experimentally on an InSb reference
|
| 795 |
+
sample. This is done by extracting Δ𝐸*+,(𝑡, 𝜏) as the difference of two separate
|
| 796 |
+
measurements of 𝐸*+,
|
| 797 |
+
&- (𝑡, 0) and 𝐸*+,
|
| 798 |
+
&..(𝑡) performed with the first lock-in amplifier and by
|
| 799 |
+
chopping only the THz probe pulse while leaving the mid-infrared pump pulse either
|
| 800 |
+
always on or always off. Equating the value of Δ𝐸*+,(𝑡, 𝜏) determined in this way to the
|
| 801 |
+
one with differential chopping yields the calibration constant.
|
| 802 |
+
|
| 803 |
+
S6. Determination of the transient optical properties
|
| 804 |
+
|
| 805 |
+
From the measured changes in the reflected probe field (see section S5), the transient
|
| 806 |
+
complex reflection coefficient of the sample 𝑟̃(𝜔, 𝜏) can be determined by taking the
|
| 807 |
+
Fourier transform along t of both 𝐸*+,
|
| 808 |
+
&..(𝑡) and Δ𝐸*+,(𝑡, 𝜏) and using the following
|
| 809 |
+
equation:
|
| 810 |
+
|
| 811 |
+
Δ𝐸:*+,(𝜔, 𝜏)
|
| 812 |
+
𝐸:*+,
|
| 813 |
+
&..(𝜔)
|
| 814 |
+
= 𝑟̃(𝜔, 𝜏) − 𝑟̃)(𝜔)
|
| 815 |
+
𝑟̃)(𝜔)
|
| 816 |
+
|
| 817 |
+
|
| 818 |
+
where 𝑟̃)(𝜔) is the equilibrium complex reflection coefficient, obtained as described in
|
| 819 |
+
section S2.
|
| 820 |
+
In the cases where the pump light penetrates in the sample several times deeper than the
|
| 821 |
+
probe light, one can assume that the probe pulse samples a volume in the material that
|
| 822 |
+
has been homogeneously excited by the pump. In this case, it is possible to directly extract
|
| 823 |
+
the complex-valued optical response functions by inverting the Fresnel equations.
|
| 824 |
+
However, in K3C60 the penetration depth of the probe electric field (~600-900 nm)
|
| 825 |
+
exceeds that of the pump (~500 nm at 10 THz, ~200 nm at 41 THz), such that the probe
|
| 826 |
+
interrogates an inhomogeneously excited volume (Figure S6.1(a)).
|
| 827 |
+
|
| 828 |
+
|
| 829 |
+
|
| 830 |
+
21
|
| 831 |
+
As the pump penetrates into the material, its intensity is reduced, and it will induce
|
| 832 |
+
progressively weaker changes in the refractive index of the sample. This situation is
|
| 833 |
+
modeled by “slicing” the probed thickness of the material into thin layers (figure S6.1(b)),
|
| 834 |
+
where we assume that the pump-induced changes in the refractive index ∆𝑛= scale
|
| 835 |
+
according to the pump intensity in the layer, i.e. 𝑛=(𝜔, 𝑧, 𝜏) = 𝑛=)(𝜔) + ∆𝑛=(𝜔, 𝜏, 𝐼(𝑧)). The
|
| 836 |
+
pump intensity 𝐼(𝑧) is assumed to follow the dependence 𝐼(𝑧) = 𝐼)𝑒2,/4!"#!, where
|
| 837 |
+
𝑑#56# = 𝜆#56# 4𝜋𝐼𝑚 D𝑛).𝜔#56#/E
|
| 838 |
+
F
|
| 839 |
+
. Here, the refractive index of the material at the
|
| 840 |
+
pump frequency, 𝑛).𝜔#56#/ is taken to be the one at equilibrium. Additionally, an
|
| 841 |
+
assumption is made on the functional form for the dependence of ∆𝑛= on the pump
|
| 842 |
+
intensity. Here, we consider two different forms given by:
|
| 843 |
+
(1) ∆𝑛=(𝜔, 𝜏, 𝑧) ∝ 𝐼(𝑧)
|
| 844 |
+
(2) ∆𝑛=(𝜔, 𝜏, 𝑧) ∝ H𝐼(𝑧)
|
| 845 |
+
Respectively, these equations result in the following depth-dependent functional forms
|
| 846 |
+
for the spatial profile of the refractive index:
|
| 847 |
+
(1) 𝑛=(𝑧, 𝜔, 𝜏) = 𝑛=)(𝜔) + Δ𝑛=(𝜔, 𝜏)𝑒2,/4!"#!
|
| 848 |
+
(2) 𝑛=(𝑧, 𝜔, 𝜏) = 𝑛=)(𝜔) + ∆𝑛=(𝜔, 𝜏)𝑒2,/"4!"#!
|
| 849 |
+
where Δ𝑛=(𝜔, 𝜏) represents the pump-induced change in the refractive index of the
|
| 850 |
+
material at the sample surface.
|
| 851 |
+
|
| 852 |
+
Figure S6.1: a. Schematics of pump-probe penetration depth mismatch. b. Multi-layer model
|
| 853 |
+
with exponential decay used to calculate the pump-induced changes in the complex refractive
|
| 854 |
+
index 𝑛#(𝜔, 𝜏) for each pump-probe delay 𝜏. The transition from red to background (grey)
|
| 855 |
+
represents the decaying pump-induced changes in 𝑛#(𝜔, 𝑧).
|
| 856 |
+
|
| 857 |
+
Sample
|
| 858 |
+
Sample
|
| 859 |
+
Probe
|
| 860 |
+
Pump
|
| 861 |
+
|
| 862 |
+
22
|
| 863 |
+
For each time delay 𝜏 and probe frequency 𝜔7, the complex reflection coefficient 𝑟̃(∆𝑛=) of
|
| 864 |
+
the multilayer stack described above is calculated using the transfer matrix method10,
|
| 865 |
+
keeping ∆𝑛= as a free parameter. To numerically extract the value of ∆𝑛=(𝜔, 𝜏) we minimize
|
| 866 |
+
the following function:
|
| 867 |
+
|
| 868 |
+
IΔ𝐸:*+,(𝜔7)
|
| 869 |
+
𝐸:*+,
|
| 870 |
+
&..(𝜔7)
|
| 871 |
+
− 𝑟̃(𝜔7, Δn) − 𝑟̃)(𝜔7)
|
| 872 |
+
𝑟̃)(𝜔7)
|
| 873 |
+
I
|
| 874 |
+
|
| 875 |
+
By then taking 𝑛=(𝜔, 𝜏) = 𝑛=)(𝜔) + Δ𝑛=(𝜔, 𝜏), one obtains the refractive index of the
|
| 876 |
+
material as if it had been homogeneously excited. From 𝑛=(𝜔, 𝜏) we then calculate 𝑅(𝜔, 𝜏),
|
| 877 |
+
𝜎!(𝜔, 𝜏) and 𝜎"(𝜔, 𝜏) as plotted in the main text.
|
| 878 |
+
Figures S6.2 and S6.3 display extended data sets measured at increasing pump-probe
|
| 879 |
+
delays with pump photon energies of 170 meV (41 THz) and 45 meV (11 THz)
|
| 880 |
+
respectively. Therein we report reflectivity (sample-diamond interface), real and
|
| 881 |
+
imaginary part of the optical conductivity after reconstruction under the assumptions of
|
| 882 |
+
models (1) and (2), identified with hollow and filled circles respectively.
|
| 883 |
+
At early delays, for both excitation mechanisms and reconstruction assumptions, the
|
| 884 |
+
reconstructed reflectivity is higher than one, and the real part of the optical conductivity
|
| 885 |
+
is negative, indicative of amplification of the incoming THz probe radiation, as discussed
|
| 886 |
+
previously in Ref. 11. In all cases, this non-equilibrium driven state then relaxes into a
|
| 887 |
+
superconducting-like state with a fully gapped 𝜎!(𝜔) and a divergence ∝ 1 𝜔
|
| 888 |
+
⁄ in the
|
| 889 |
+
𝜎"(𝜔) spectrum. At even later delays the optical spectra are those of a finite temperature
|
| 890 |
+
superconductor. These optical properties can be interpreted in the context of a two fluid
|
| 891 |
+
model, in which a varying density of uncondensed quasi-particles also contributes to the
|
| 892 |
+
terahertz response.
|
| 893 |
+
Importantly the time-evolution of K3C60 following photo-excitation is independent of the
|
| 894 |
+
used reconstruction, and only the specific values of pump-probe delay up to which
|
| 895 |
+
amplification, fully gapped superconductor, and finite temperature superconductor
|
| 896 |
+
appear are affected by this choice.
|
| 897 |
+
|
| 898 |
+
|
| 899 |
+
|
| 900 |
+
23
|
| 901 |
+
|
| 902 |
+
Figure S6.2: Comparison of linear and sub-linear reconstruction in the transient optical spectra
|
| 903 |
+
at 170 meV (41 THz) pump-photon energy. Reflectivity (sample-diamond interface), real, and
|
| 904 |
+
imaginary parts of the optical conductivity measured at equilibrium (red lines) and after
|
| 905 |
+
photoexcitation (blue symbols) at increasing pump-probe time delays indicated in the figure. The data
|
| 906 |
+
in filled (open) symbols reconstructed under the assumption of a square-root (linear) fluence
|
| 907 |
+
dependence of the changes in complex refractive index of the material. These data were measured at
|
| 908 |
+
18 mJ cm-2 excitation fluence, and at a base temperature of 100 K.
|
| 909 |
+
|
| 910 |
+
0 ps
|
| 911 |
+
1 ps
|
| 912 |
+
2 ps
|
| 913 |
+
5 ps
|
| 914 |
+
10 ps
|
| 915 |
+
50 ps
|
| 916 |
+
|
| 917 |
+
24
|
| 918 |
+
|
| 919 |
+
Figure S6.3: Comparison of linear and sub-linear reconstruction in the transient optical spectra
|
| 920 |
+
at 45 meV (11 THz) pump-photon energy. Reflectivity (sample-diamond interface), real, and
|
| 921 |
+
imaginary parts of the optical conductivity measured at equilibrium (red lines) and after
|
| 922 |
+
photoexcitation (blue symbols) at increasing pump-probe time delays indicated in the figure. The data
|
| 923 |
+
in filled (open) symbols reconstructed under the assumption of a square-root (linear) fluence
|
| 924 |
+
dependence of the changes in complex refractive index of the material. These data were measured at
|
| 925 |
+
0.5 mJ cm-2 excitation fluence, and at a base temperature of 100 K.
|
| 926 |
+
|
| 927 |
+
1.5 ps
|
| 928 |
+
3.5 ps
|
| 929 |
+
5.5 ps
|
| 930 |
+
11.5 ps
|
| 931 |
+
50.5 ps
|
| 932 |
+
|
| 933 |
+
25
|
| 934 |
+
S7. Fitting of the transient optical spectra
|
| 935 |
+
|
| 936 |
+
The transient optical conductivity spectra presented in figures 2-3 as well as for each
|
| 937 |
+
fluence in figure 4 were fitted with a two-fluid model according to the following equation:
|
| 938 |
+
𝜎=(𝜔, 𝜏) = 𝜋
|
| 939 |
+
2
|
| 940 |
+
Λ'(𝜏) 𝑒"
|
| 941 |
+
𝑚
|
| 942 |
+
𝛿[𝜔 = 0] + 𝑖 Λ'(𝜏) 𝑒"
|
| 943 |
+
𝑚
|
| 944 |
+
1
|
| 945 |
+
𝜔
|
| 946 |
+
+ Λ-(𝜏) 𝑒"
|
| 947 |
+
𝑚
|
| 948 |
+
1
|
| 949 |
+
𝛾$ − 𝑖𝜔
|
| 950 |
+
+ R
|
| 951 |
+
𝐵-𝜔
|
| 952 |
+
𝑖(Ω-" − 𝜔") + 𝛾-𝜔
|
| 953 |
+
"
|
| 954 |
+
-8!
|
| 955 |
+
|
| 956 |
+
|
| 957 |
+
Here the first term captures the frequency dependent contribution from the
|
| 958 |
+
supercarriers with density Λ', the second term captures the Drude contribution of the
|
| 959 |
+
normal carriers with density Λ- and scattering rate 𝛾$. Finally, we include a sum over
|
| 960 |
+
|
| 961 |
+
Figure S7.1: Two-fluid fit to the transient spectrum. Reflectivity, real (𝜎!) and imaginary (𝜎")
|
| 962 |
+
parts of the optical conductivity measured in equilibrium at 100 K (red) and 50 ps after
|
| 963 |
+
photoexcitation with a fluence of 0.5 mJ cm-2 at 45 meV (11 THz) photon energy. The fit to the
|
| 964 |
+
equilibrium data using the procedure described in this section is shown as a dashed black line and
|
| 965 |
+
gives zero superfluid density. The two-fluid fit to the transient data generated using the same
|
| 966 |
+
procedure is shown as a solid blue line and returns a superfluid fraction Λ# (Λ$ + Λ#)
|
| 967 |
+
⁄
|
| 968 |
+
= 73%. The
|
| 969 |
+
data in this figure was reconstructed under the assumption of a square root dependence of the
|
| 970 |
+
change in refractive index on excitation fluence (see supplementary section S6).
|
| 971 |
+
|
| 972 |
+
|
| 973 |
+
|
| 974 |
+
26
|
| 975 |
+
two Lorentz oscillators in order to capture the broad midinfrared absorption peak
|
| 976 |
+
centered at around 60 meV.
|
| 977 |
+
The transient data are fitted at each delay 𝜏 using the parameter-set that captures the
|
| 978 |
+
equilibrium optical conductivity spectra as a starting condition, and leaving only Λ' and
|
| 979 |
+
Λ- free to vary, as though the effect of the pump is to simply convert carriers from the
|
| 980 |
+
normal to the superconducting fluid.
|
| 981 |
+
Figure S7.1 shows representative fits to transient data measured at 100 K base
|
| 982 |
+
temperature and at 50 ps time delay, as well as to the 100 K equilibrium spectra.
|
| 983 |
+
Importantly, while the fit of the equilibrium data converges to a superfluid fraction
|
| 984 |
+
Λ' (Λ- + Λ')
|
| 985 |
+
⁄
|
| 986 |
+
which is equal to zero, the fit to the transient data yields Λ' (Λ-
|
| 987 |
+
⁄
|
| 988 |
+
+ Λ') =
|
| 989 |
+
0.73. The transient optical data was fitted at each time delay and driving frequency,
|
| 990 |
+
yielding the time and frequency dependence of the superfluid fractions shown in figures
|
| 991 |
+
2(e), 3(e), and 4(a).
|
| 992 |
+
|
| 993 |
+
S8. Extracting the frequency-dependent photosusceptibility
|
| 994 |
+
|
| 995 |
+
In figure 4(b) we introduce a figure of merit, referred to as the ‘photosusceptibility’,
|
| 996 |
+
which can be used to quantitatively compare the efficiency with which the metastable
|
| 997 |
+
light-induced superconducting state is generated in K3C60 for different excitation
|
| 998 |
+
frequencies.
|
| 999 |
+
For each excitation photon energy, transient optical spectra were measured at different
|
| 1000 |
+
excitation fluences ℱ. From these fluence dependent spectra we extract the loss in
|
| 1001 |
+
spectral weight of 𝜎!(𝜔) after photoexcitation in the 5-10 meV spectral range, calculated
|
| 1002 |
+
as:
|
| 1003 |
+
𝑆𝑊𝐿(ℱ) = Z
|
| 1004 |
+
𝜎!
|
| 1005 |
+
9:(𝜔) − 𝜎!
|
| 1006 |
+
#;&<&(𝜔, ℱ) 𝑑𝜔
|
| 1007 |
+
!) meV/ℏ
|
| 1008 |
+
B meV/ℏ
|
| 1009 |
+
|
| 1010 |
+
where 𝜎!
|
| 1011 |
+
9:(𝜔) and 𝜎!
|
| 1012 |
+
#;&<&(𝜔, ℱ) are the 𝜎!(𝜔) spectra measured in equilibrium and upon
|
| 1013 |
+
photoexcitation respectively. The 𝑆𝑊𝐿(ℱ) data is then fitted with the following
|
| 1014 |
+
phenomenological function:
|
| 1015 |
+
𝐴 \
|
| 1016 |
+
1
|
| 1017 |
+
1 + 𝐵𝑒2CDℱ
|
| 1018 |
+
1
|
| 1019 |
+
− 1
|
| 1020 |
+
2]
|
| 1021 |
+
|
| 1022 |
+
|
| 1023 |
+
|
| 1024 |
+
27
|
| 1025 |
+
where ℱ represents the excitation fluence and 𝐴, 𝐵 are free parameters. The
|
| 1026 |
+
‘photosusceptibility’ plotted in figure 4(b) is equal to 𝐵, which is the gradient of this
|
| 1027 |
+
function evaluated at zero fluence. Figure S8.1 shows the fluence-dependent data and
|
| 1028 |
+
corresponding fit for one exemplary dataset.
|
| 1029 |
+
|
| 1030 |
+
Figure S8.1: Extracting photosusceptibility from the fluence-dependent data. Lost spectral
|
| 1031 |
+
weight in the real part of the optical conductivity between 5 and 10 meV as a function of fluence (red
|
| 1032 |
+
circles), measured 10 ps after photoexcitation at 100 K with a pump spectrum centered at 41 meV (10
|
| 1033 |
+
THz). The fit is shown as a solid green line, with the gradient at zero fluence (which we define as the
|
| 1034 |
+
photosusceptibility) shown as a dashed blue line. The data in this figure was reconstructed under the
|
| 1035 |
+
assumption of a square root dependence of the change in refractive index on excitation fluence (see
|
| 1036 |
+
supplementary section S6).
|
| 1037 |
+
|
| 1038 |
+
S9. Density functional theory calculations
|
| 1039 |
+
|
| 1040 |
+
In this section, we address how the displacement of phonon modes affects the electronic
|
| 1041 |
+
properties of K3C60. Specifically, we consider the molecular orbitals and their response to
|
| 1042 |
+
the change in the crystal structure. To carry out this investigation, a first-principles
|
| 1043 |
+
approach based on density functional theory (DFT) was used. The starting point is the
|
| 1044 |
+
unit cell of K3C60 containing sixty carbon and three potassium atoms. Before computing
|
| 1045 |
+
|
| 1046 |
+
|
| 1047 |
+
|
| 1048 |
+
28
|
| 1049 |
+
the phonon spectrum, this unit cell is structurally relaxed, and the resulting lattice
|
| 1050 |
+
constants and atomic coordinates are listed in table S9.1.
|
| 1051 |
+
Next, the phonon spectrum of K3C60 is computed from the force constant matrix utilizing
|
| 1052 |
+
a finite displacement approach12. In total, there are 186 non-translational phonon modes
|
| 1053 |
+
covering the symmetries of point group m-3. Specifically, there are 24 Tu, 7 Eu, 23 Tg, 8 Eg,
|
| 1054 |
+
and 8 Ag modes. Note that only the modes of Tu character are infrared active, and we list
|
| 1055 |
+
their computed frequencies in the table S9.2.
|
| 1056 |
+
We utilized a frozen phonon approach to estimate the impact of these distortions on the
|
| 1057 |
+
molecular levels. Therefore, we modulated our equilibrium crystal structure with the
|
| 1058 |
+
eigen-displacements of these modes. We then created a low energy Hamiltonian for these
|
| 1059 |
+
structures by computing the maximally localized Wannier functions for the valence band
|
| 1060 |
+
electrons. Note that since the three valence bands are well separated in energy from other
|
| 1061 |
+
orbital-like bands our method does not require a disentanglement procedure.
|
| 1062 |
+
Our calculations focused on the three degenerate t1u molecular levels at the Fermi energy,
|
| 1063 |
+
which we mapped out from DFT wave functions as maximally-localized Wannier
|
| 1064 |
+
functions. In the equilibrium structure, the onsite energy of these molecular levels is
|
| 1065 |
+
degenerate; however, deforming the crystal by applying a T1u polar distortion lifts this
|
| 1066 |
+
degeneracy. Thereby, similar to a Jahn-Teller distortion, the symmetry breaking of the
|
| 1067 |
+
crystal structure splits the level into a double and a single degenerate orbital. For the 43.2
|
| 1068 |
+
meV and 173.4 meV phonon modes, this splitting manifests as a lowering in the energy
|
| 1069 |
+
of the double degenerate orbital. A schematic visualization of this is depicted in the inset
|
| 1070 |
+
to figure S9.1(a). Diagrams illustrating the distortion of the C60 molecule for the 43.2 meV
|
| 1071 |
+
Lattice vectors
|
| 1072 |
+
a
|
| 1073 |
+
14.175 Å
|
| 1074 |
+
Alpha
|
| 1075 |
+
90˚
|
| 1076 |
+
90˚
|
| 1077 |
+
90˚
|
| 1078 |
+
b
|
| 1079 |
+
14.175 Å
|
| 1080 |
+
Beta
|
| 1081 |
+
c
|
| 1082 |
+
14.175 Å
|
| 1083 |
+
Gamma
|
| 1084 |
+
Atomic positions according to Space Group 202 (Fm-3)
|
| 1085 |
+
Element
|
| 1086 |
+
Wykoff label
|
| 1087 |
+
X
|
| 1088 |
+
y
|
| 1089 |
+
c
|
| 1090 |
+
C
|
| 1091 |
+
H
|
| 1092 |
+
0.00000
|
| 1093 |
+
0.54991
|
| 1094 |
+
0.24682
|
| 1095 |
+
C
|
| 1096 |
+
I
|
| 1097 |
+
0.58242
|
| 1098 |
+
0.10057
|
| 1099 |
+
0.21408
|
| 1100 |
+
C
|
| 1101 |
+
I
|
| 1102 |
+
0.66275
|
| 1103 |
+
0.05092
|
| 1104 |
+
0.18294
|
| 1105 |
+
K
|
| 1106 |
+
C
|
| 1107 |
+
0.25000
|
| 1108 |
+
0.25000
|
| 1109 |
+
0.25000
|
| 1110 |
+
K
|
| 1111 |
+
A
|
| 1112 |
+
0.00000
|
| 1113 |
+
0.00000
|
| 1114 |
+
0.00000
|
| 1115 |
+
|
| 1116 |
+
Table S9.1: Structural parameters of K3C60 from first-principles computations
|
| 1117 |
+
|
| 1118 |
+
|
| 1119 |
+
|
| 1120 |
+
29
|
| 1121 |
+
and 173.4 meV modes (labelled ‘A’ and ‘B’ and corresponding to mode numbers 4 and 21
|
| 1122 |
+
in table S9.2 respectively) are shown in figure S9.1(b).
|
| 1123 |
+
Besides this qualitative difference of the phonon-mode distortion on the molecular levels,
|
| 1124 |
+
we also examined the strength of the induced splitting. From group-theory, the size of the
|
| 1125 |
+
splitting scales with the square of the distortion. Figure S9.1(a) displays how the splitting
|
| 1126 |
+
develops as a function of the fluence of the incoming THz pulse. Each phonon mode
|
| 1127 |
+
distortion was weighted according to its eigenfrequency and mode effective charge in this
|
| 1128 |
+
plot. For the same strength of the driving electric field, the splitting induced by phonon
|
| 1129 |
+
A produces a more significant separation of the t1u levels compared to phonon B. Due to
|
| 1130 |
+
the square scaling of the splitting with the electric field, this effect is further enhanced at
|
| 1131 |
+
higher field strengths.
|
| 1132 |
+
The computations were performed with the Vienna ab-initio simulation package
|
| 1133 |
+
VASP.6.213-15. For the phonon calculations, we used the Phonopy software package16 and
|
| 1134 |
+
the Wannier90 package for wannierization12. The computations further utilized
|
| 1135 |
+
Number:
|
| 1136 |
+
ℎ𝜈#56# (meV)
|
| 1137 |
+
1
|
| 1138 |
+
2.2
|
| 1139 |
+
2
|
| 1140 |
+
14.1
|
| 1141 |
+
3
|
| 1142 |
+
42.4
|
| 1143 |
+
4 (A)
|
| 1144 |
+
43.2
|
| 1145 |
+
5
|
| 1146 |
+
48.3
|
| 1147 |
+
6
|
| 1148 |
+
60.5
|
| 1149 |
+
7
|
| 1150 |
+
62.6
|
| 1151 |
+
8
|
| 1152 |
+
71.5
|
| 1153 |
+
9
|
| 1154 |
+
80.6
|
| 1155 |
+
10
|
| 1156 |
+
83.9
|
| 1157 |
+
11
|
| 1158 |
+
85.9
|
| 1159 |
+
12
|
| 1160 |
+
91.1
|
| 1161 |
+
13
|
| 1162 |
+
92.0
|
| 1163 |
+
14
|
| 1164 |
+
118.6
|
| 1165 |
+
15
|
| 1166 |
+
122.8
|
| 1167 |
+
16
|
| 1168 |
+
147.5
|
| 1169 |
+
17
|
| 1170 |
+
148.3
|
| 1171 |
+
18
|
| 1172 |
+
149.8
|
| 1173 |
+
19
|
| 1174 |
+
163.7
|
| 1175 |
+
20
|
| 1176 |
+
165.4
|
| 1177 |
+
21 (B)
|
| 1178 |
+
173.4
|
| 1179 |
+
22
|
| 1180 |
+
176.9
|
| 1181 |
+
23
|
| 1182 |
+
184.8
|
| 1183 |
+
24
|
| 1184 |
+
185.3
|
| 1185 |
+
|
| 1186 |
+
Table S9.2: List of the IR active phonon modes of Tu symmetry.
|
| 1187 |
+
|
| 1188 |
+
|
| 1189 |
+
|
| 1190 |
+
30
|
| 1191 |
+
pseudopotentials generated within the Projected Augmented Wave (PAW) method16.
|
| 1192 |
+
Specifically, the following default potentials were used: C 2s22p2 and K 3s23p64s1. The
|
| 1193 |
+
Generalized Gradient Approximation (GGA17) approximation for the exchange-
|
| 1194 |
+
correlation potential was used. For the final numerical setting, a 4x4x4 Monkhorst18
|
| 1195 |
+
generated k-point-mesh sampling of the Brillouin zone and a plane-wave energy cutoff of
|
| 1196 |
+
600 eV were chosen. The calculations were re-iterated self-consistently until the change
|
| 1197 |
+
in total energy converged within 10-8 eV.
|
| 1198 |
+
|
| 1199 |
+
|
| 1200 |
+
Figure S9.1: Effect of vibrational distortions on the t1u molecular levels from first-principle
|
| 1201 |
+
computations. (a) shows the induced splitting of the molecular orbital of t1u symmetry at the Fermi
|
| 1202 |
+
energy (as illustrated by the inset) as a function of drive fluence. The two curves represent the effect
|
| 1203 |
+
of the two distinct T1u IR-phonon modes with eigenfrequencies of 43.2 (red) and 173.4 (blue) meV.
|
| 1204 |
+
The eigen displacement of these modes are shown in (b). Note, that due to the symmetry character of
|
| 1205 |
+
the phonon modes the t1u level split into a single and double degenerate orbital. Lastly, in (c) we show
|
| 1206 |
+
the induced splitting as a function of frequency for a fixed fluence. Here we consider the whole
|
| 1207 |
+
spectrum of T1u IR modes of K3C60, as listed in table S9.2.
|
| 1208 |
+
|
| 1209 |
+
S10. Local electronic hamiltonian calculations
|
| 1210 |
+
|
| 1211 |
+
The Hamiltonian proposed in Ref. 19 in order to model superconductivity in alkali-doped
|
| 1212 |
+
fullerides is based on an effective negative Hund’s coupling J. It arises from a combination of
|
| 1213 |
+
the usual Hund’s coupling with a dynamical Jahn-Teller distortion. This causes states featuring
|
| 1214 |
+
intra-orbital pairing on a buckyball to be energetically favourable. Using ab-initio calculations,
|
| 1215 |
+
|
| 1216 |
+
B
|
| 1217 |
+
|
| 1218 |
+
31
|
| 1219 |
+
values of the intra-orbital interaction U = 0.826 eV and of J = −18.5meV were predicted for
|
| 1220 |
+
K3C6020. The phase diagram for the A3C60 family of compounds was computed using DMFT
|
| 1221 |
+
starting from this Hamiltonian and was found to be in quantitative agreement with experimental
|
| 1222 |
+
data21.
|
| 1223 |
+
The Hamiltonian can be written as:
|
| 1224 |
+
|
| 1225 |
+
𝐻 = 𝐻Intra + 𝐻Inter + 𝐻Pairhop + 𝐻Spinswap
|
| 1226 |
+
|
| 1227 |
+
with an intra-orbital interaction with magnitude U given by:
|
| 1228 |
+
|
| 1229 |
+
𝐻Intra = 𝑈 R 𝑛7,↑𝑛7,↓
|
| 1230 |
+
U
|
| 1231 |
+
7
|
| 1232 |
+
|
| 1233 |
+
|
| 1234 |
+
where 𝑛7,V = 𝑎7,V
|
| 1235 |
+
W 𝑎7,V is the number operator for a spin down electron on orbital i with spin 𝜎 ∈
|
| 1236 |
+
{↑, ↓}. 𝑎7,V
|
| 1237 |
+
W and 𝑎7,V are fermion creation and annihilation operators, respectively. The inter-
|
| 1238 |
+
orbital interaction appears as:
|
| 1239 |
+
|
| 1240 |
+
𝐻Inter = (𝑈 − 2𝐽) R R .1 − δ7X/𝑛7,↑𝑛X,↓
|
| 1241 |
+
U
|
| 1242 |
+
X
|
| 1243 |
+
U
|
| 1244 |
+
7
|
| 1245 |
+
+ (𝑈 − 3𝐽) R R R
|
| 1246 |
+
𝑛7,V𝑛X,V
|
| 1247 |
+
72!
|
| 1248 |
+
X
|
| 1249 |
+
U
|
| 1250 |
+
7
|
| 1251 |
+
V
|
| 1252 |
+
|
| 1253 |
+
|
| 1254 |
+
with δ7X denoting the Kronecker delta. which, given that J is negative, makes these terms higher
|
| 1255 |
+
in energy. In addition, there is a pair hopping term, which corresponds to a transfer of a pair of
|
| 1256 |
+
electrons from one orbital to another. It is given by:
|
| 1257 |
+
|
| 1258 |
+
𝐻Pairhop = 𝐽 R R .1 − δ7X/𝑎7,↑
|
| 1259 |
+
W 𝑎7,↓
|
| 1260 |
+
W 𝑎X,↓𝑎X,↑
|
| 1261 |
+
U
|
| 1262 |
+
X
|
| 1263 |
+
U
|
| 1264 |
+
7
|
| 1265 |
+
|
| 1266 |
+
|
| 1267 |
+
This term was found to be crucial for the appearance of superconductivity21. Finally, there is a
|
| 1268 |
+
“spin
|
| 1269 |
+
swapping”
|
| 1270 |
+
term,
|
| 1271 |
+
where
|
| 1272 |
+
two
|
| 1273 |
+
opposite
|
| 1274 |
+
spins
|
| 1275 |
+
exchange
|
| 1276 |
+
orbitals:
|
| 1277 |
+
|
| 1278 |
+
−𝐽 R R .1 − δ7X/𝑎7,↑
|
| 1279 |
+
W 𝑎7,↓𝑎X,↓
|
| 1280 |
+
W 𝑎X,↑
|
| 1281 |
+
U
|
| 1282 |
+
X
|
| 1283 |
+
U
|
| 1284 |
+
7
|
| 1285 |
+
|
| 1286 |
+
|
| 1287 |
+
|
| 1288 |
+
|
| 1289 |
+
|
| 1290 |
+
32
|
| 1291 |
+
When restricting ourselves to a Hilbert space where the three degenerate orbitals are populated
|
| 1292 |
+
by three electrons (as is appropriate for A3C60 in the atomic limit), we can use a basis given by
|
| 1293 |
+
the different possible arrangements in which the orbitals can be populated:
|
| 1294 |
+
|
| 1295 |
+
{|↑, ↑↓ ,0⟩,|↑ ,0, ↑↓⟩,|↑↓, ↑ ,0⟩,|0, ↑, ↑↓⟩,|↑↓ ,0, ↑⟩,|0, ↑↓, ↑⟩, |↓, ↑, ↑⟩,|↑, ↓, ↑⟩,|↑, ↑, ↓⟩,|↑, ↑, ↑⟩}
|
| 1296 |
+
|
| 1297 |
+
as well as a second set of states created by flipping all spins in the set above.
|
| 1298 |
+
In this basis, the Hamiltonian takes on the form:
|
| 1299 |
+
|
| 1300 |
+
𝐻m − (3𝑈 + 5𝐽)𝐼o = −𝐽
|
| 1301 |
+
⎝
|
| 1302 |
+
⎜
|
| 1303 |
+
⎜
|
| 1304 |
+
⎜
|
| 1305 |
+
⎜
|
| 1306 |
+
⎜
|
| 1307 |
+
⎜
|
| 1308 |
+
⎛
|
| 1309 |
+
0
|
| 1310 |
+
−1
|
| 1311 |
+
0
|
| 1312 |
+
0
|
| 1313 |
+
0
|
| 1314 |
+
0
|
| 1315 |
+
0
|
| 1316 |
+
0
|
| 1317 |
+
0
|
| 1318 |
+
0
|
| 1319 |
+
−1
|
| 1320 |
+
0
|
| 1321 |
+
0
|
| 1322 |
+
0
|
| 1323 |
+
0
|
| 1324 |
+
0
|
| 1325 |
+
0
|
| 1326 |
+
0
|
| 1327 |
+
0
|
| 1328 |
+
0
|
| 1329 |
+
0
|
| 1330 |
+
0
|
| 1331 |
+
0
|
| 1332 |
+
+1
|
| 1333 |
+
0
|
| 1334 |
+
0
|
| 1335 |
+
0
|
| 1336 |
+
0
|
| 1337 |
+
0
|
| 1338 |
+
0
|
| 1339 |
+
0
|
| 1340 |
+
0
|
| 1341 |
+
+1
|
| 1342 |
+
0
|
| 1343 |
+
0
|
| 1344 |
+
0
|
| 1345 |
+
0
|
| 1346 |
+
0
|
| 1347 |
+
0
|
| 1348 |
+
0
|
| 1349 |
+
0
|
| 1350 |
+
0
|
| 1351 |
+
0
|
| 1352 |
+
0
|
| 1353 |
+
0
|
| 1354 |
+
−1
|
| 1355 |
+
0
|
| 1356 |
+
0
|
| 1357 |
+
0
|
| 1358 |
+
0
|
| 1359 |
+
0
|
| 1360 |
+
0
|
| 1361 |
+
0
|
| 1362 |
+
0
|
| 1363 |
+
−1
|
| 1364 |
+
0
|
| 1365 |
+
0
|
| 1366 |
+
0
|
| 1367 |
+
0
|
| 1368 |
+
0
|
| 1369 |
+
0
|
| 1370 |
+
0
|
| 1371 |
+
0
|
| 1372 |
+
0
|
| 1373 |
+
0
|
| 1374 |
+
0
|
| 1375 |
+
+2
|
| 1376 |
+
−1
|
| 1377 |
+
+1
|
| 1378 |
+
0
|
| 1379 |
+
0
|
| 1380 |
+
0
|
| 1381 |
+
0
|
| 1382 |
+
0
|
| 1383 |
+
0
|
| 1384 |
+
0
|
| 1385 |
+
−1
|
| 1386 |
+
+2
|
| 1387 |
+
−1
|
| 1388 |
+
0
|
| 1389 |
+
0
|
| 1390 |
+
0
|
| 1391 |
+
0
|
| 1392 |
+
0
|
| 1393 |
+
0
|
| 1394 |
+
0
|
| 1395 |
+
+1
|
| 1396 |
+
−1
|
| 1397 |
+
+2
|
| 1398 |
+
0
|
| 1399 |
+
0
|
| 1400 |
+
0
|
| 1401 |
+
0
|
| 1402 |
+
0
|
| 1403 |
+
0
|
| 1404 |
+
0
|
| 1405 |
+
0
|
| 1406 |
+
0
|
| 1407 |
+
0
|
| 1408 |
+
+4⎠
|
| 1409 |
+
⎟
|
| 1410 |
+
⎟
|
| 1411 |
+
⎟
|
| 1412 |
+
⎟
|
| 1413 |
+
⎟
|
| 1414 |
+
⎟
|
| 1415 |
+
⎞
|
| 1416 |
+
|
| 1417 |
+
|
| 1418 |
+
where 𝐼o is the identity matrix, which encodes an overall energy offset. This matrix is block-
|
| 1419 |
+
diagonal, meaning that different sectors of the Hilbert space are not coupled to each other: For
|
| 1420 |
+
example, there is no term that destroys or creates pairs. Because of the inverted Hund’s
|
| 1421 |
+
coupling, i.e. because J is negative, the stretched state |↑, ↑, ↑⟩ as well as its global spin-flip
|
| 1422 |
+
partner |↓, ↓, ↓⟩ are now the most energetic local eigenstates.
|
| 1423 |
+
The local ground state is 6-fold degenerate, with an exemplary instance given by:
|
| 1424 |
+
|𝑔!⟩ = (|↑, ↑↓ ,0⟩ +|↑ ,0, ↑↓⟩)/√2, i.e. it is a state where one singlet pair of electrons has de-
|
| 1425 |
+
localized over two orbitals.
|
| 1426 |
+
The first excited manifold is 10-fold degenerate. Six of those states are of the type
|
| 1427 |
+
|𝑒!⟩ = ((|↑, ↑↓ ,0⟩ −|↑ ,0, ↑↓⟩)/√2 i.e. identical to the ground state except for the phase of the
|
| 1428 |
+
de-localized singlet pair (and hence corresponding to a different local angular momentum) –
|
| 1429 |
+
as illustrated in Figure S10.1.
|
| 1430 |
+
The energy difference between these two manifolds is given by 2J=37meV, remarkably close
|
| 1431 |
+
to the observed resonance in the experiment. However, several questions remain in order to
|
| 1432 |
+
determine whether an excitation of this transition is responsible for the experimental
|
| 1433 |
+
observation:
|
| 1434 |
+
|
| 1435 |
+
|
| 1436 |
+
|
| 1437 |
+
33
|
| 1438 |
+
Firstly, how does the light field of the laser couple to
|
| 1439 |
+
this excitation? As the size of a buckyball is
|
| 1440 |
+
comparable to the distance between buckyballs both
|
| 1441 |
+
inter-site and intra-site driving terms may be
|
| 1442 |
+
comparable in terms of the associated energy.
|
| 1443 |
+
Understanding possible inter-site driving terms
|
| 1444 |
+
(arising from the oscillating energy difference
|
| 1445 |
+
between neighbouring sites, given by the electric
|
| 1446 |
+
field multiplied with the charge and the lattice
|
| 1447 |
+
spacing) will require a calculation featuring multiple
|
| 1448 |
+
buckyballs. Locally, because the dynamical Jahn-
|
| 1449 |
+
Teller distortion causes the populated orbitals to be
|
| 1450 |
+
superpositions of several undistorted orbitals, we
|
| 1451 |
+
may expect the electric field to lift the orbital
|
| 1452 |
+
degeneracy, for example through an orbital offset
|
| 1453 |
+
term of the type 𝐻offset = Δ(𝑛U,↑ + 𝑛U,↓), where Δ
|
| 1454 |
+
encodes the amplitude of the drive and is oscillating
|
| 1455 |
+
in time. Such a term would in fact cause an excitation from |𝑒!⟩ to |𝑔!⟩, but it would not
|
| 1456 |
+
populate any un-paired state (which are not affected by this driving term, as all orbitals are
|
| 1457 |
+
equally occupied).
|
| 1458 |
+
Secondly, K3C60 has an electronic bandwidth of about 0.5eV21, meaning that the system is far
|
| 1459 |
+
away from the atomic limit (i.e. zero inter-site tunneling). Nevertheless, because the excitation
|
| 1460 |
+
here does not require inter-site tunneling (unlike e.g., double occupancy creation in a regular
|
| 1461 |
+
one-band Hubbard model), it may remain sufficiently separable.
|
| 1462 |
+
Finally, how does this excitation generate superconductivity? Indeed, the Suhl-Kondo
|
| 1463 |
+
mechanism suggests that in a multi-band system, pairs in any local superposition can contribute
|
| 1464 |
+
to superconductivity, but how the generation of excited-state pairs can lead to superconducting
|
| 1465 |
+
properties starting from a normal state remains to be investigated.
|
| 1466 |
+
|
| 1467 |
+
|
| 1468 |
+
Figure S10.1: Ground state and first
|
| 1469 |
+
excited state of the local Hamiltonian.
|
| 1470 |
+
The yellow lines indicate the phase of the
|
| 1471 |
+
pair which is de-localized over two
|
| 1472 |
+
orbitals. The energy spacing between
|
| 1473 |
+
these two states is given by -2J
|
| 1474 |
+
|
| 1475 |
+
-2J
|
| 1476 |
+
|
| 1477 |
+
34
|
| 1478 |
+
References
|
| 1479 |
+
1
|
| 1480 |
+
Mitrano, M. et al. Possible light-induced superconductivity in K3C60 at high temperature.
|
| 1481 |
+
Nature 530, 461-464, (2016).
|
| 1482 |
+
2
|
| 1483 |
+
Cantaluppi, A. et al. Pressure tuning of light-induced superconductivity in K3C60. Nature
|
| 1484 |
+
Physics 14, 837-841, (2018).
|
| 1485 |
+
3
|
| 1486 |
+
Budden, M. et al. Evidence for metastable photo-induced superconductivity in K3C60.
|
| 1487 |
+
Nature Physics 17, 611-618, (2021).
|
| 1488 |
+
4
|
| 1489 |
+
Plaskett, J. S. & Schatz, P. N. On the Robinson and Price (Kramers—Kronig) Method of
|
| 1490 |
+
Interpreting Reflection Data Taken through a Transparent Window. The Journal of
|
| 1491 |
+
Chemical Physics 38, 612-617, (1963).
|
| 1492 |
+
5
|
| 1493 |
+
Degiorgi, L. et al. Optical properties of the alkali-metal-doped superconducting fullerenes:
|
| 1494 |
+
K3C60 and Rb3C60. Physical Review B 49, 7012-7025, (1994).
|
| 1495 |
+
6
|
| 1496 |
+
Degiorgi, L., Briceno, G., Fuhrer, M. S., Zettl, A. & Wachter, P. Optical measurements of the
|
| 1497 |
+
superconducting gap in single-crystal K3C60 and Rb3C60. Nature 369, 541-543, (1994).
|
| 1498 |
+
7
|
| 1499 |
+
Liu, B. et al. Generation of narrowband, high-intensity, carrier-envelope phase-stable
|
| 1500 |
+
pulses tunable between 4 and 18 THz. Opt. Lett. 42, 129-131, (2017).
|
| 1501 |
+
8
|
| 1502 |
+
Kindt, J. T. & Schmuttenmaer, C. A. Theory for determination of the low-frequency time-
|
| 1503 |
+
dependent response function in liquids using time-resolved terahertz pulse spectroscopy.
|
| 1504 |
+
The Journal of Chemical Physics 110, 8589-8596, (1999).
|
| 1505 |
+
9
|
| 1506 |
+
Schmuttenmaer, C. A. Exploring Dynamics in the Far-Infrared with Terahertz
|
| 1507 |
+
Spectroscopy. Chemical Reviews 104, 1759-1780, (2004).
|
| 1508 |
+
10
|
| 1509 |
+
Born, M. & Wolf, E. Principles of Optics. 7th edn, (Cambridge University Press, 1999).
|
| 1510 |
+
11
|
| 1511 |
+
Buzzi, M. et al. Higgs-Mediated Optical Amplification in a Nonequilibrium Superconductor.
|
| 1512 |
+
Physical Review X 11, 011055, (2021).
|
| 1513 |
+
12
|
| 1514 |
+
Marzari, N. & Vanderbilt, D. Maximally localized generalized Wannier functions for
|
| 1515 |
+
composite energy bands. Physical Review B 56, 12847-12865, (1997).
|
| 1516 |
+
|
| 1517 |
+
|
| 1518 |
+
|
| 1519 |
+
35
|
| 1520 |
+
13
|
| 1521 |
+
Kresse, G. & Furthmüller, J. Efficiency of ab-initio total energy calculations for metals and
|
| 1522 |
+
semiconductors using a plane-wave basis set. Computational Materials Science 6, 15-50,
|
| 1523 |
+
(1996).
|
| 1524 |
+
14
|
| 1525 |
+
Kresse, G. & Hafner, J. Ab initio molecular dynamics for open-shell transition metals.
|
| 1526 |
+
Physical Review B 48, 13115-13118, (1993).
|
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|
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|
| 1549 |
+
|
| 1550 |
+
|
7dFAT4oBgHgl3EQfoR1F/content/tmp_files/load_file.txt
ADDED
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See raw diff
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7tAzT4oBgHgl3EQfgfwd/content/tmp_files/2301.01468v1.pdf.txt
ADDED
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|
| 1 |
+
Black hole interiors
|
| 2 |
+
in holographic topological semimetals
|
| 3 |
+
Ling-Long Gao a,b1, Yan Liu a,b2 and Hong-Da Lyu a,b3
|
| 4 |
+
aCenter for Gravitational Physics, Department of Space Science
|
| 5 |
+
and International Research Institute of Multidisciplinary Science,
|
| 6 |
+
Beihang University, Beijing 100191, China
|
| 7 |
+
bPeng Huanwu Collaborative Center for Research and Education,
|
| 8 |
+
Beihang University, Beijing 100191, China
|
| 9 |
+
Abstract
|
| 10 |
+
We study the black hole interiors in holographic Weyl semimetals and holo-
|
| 11 |
+
graphic nodal line semimetals.
|
| 12 |
+
We find that the black hole singularities are of
|
| 13 |
+
Kasner form. In the topologically nontrivial phase at low temperature, both the
|
| 14 |
+
Kasner exponents of the metric fields and the proper time from the horizon to the
|
| 15 |
+
singularity are almost constant, likely reflecting the topological nature of the topo-
|
| 16 |
+
logical semimetals. We also find some specific behaviors inside the horizon in each
|
| 17 |
+
holographic semimetal model.
|
| 18 |
+
1Email: linglonggao@buaa.edu.cn
|
| 19 |
+
2Email: yanliu@buaa.edu.cn
|
| 20 |
+
3Email: hongdalyu@buaa.edu.cn
|
| 21 |
+
arXiv:2301.01468v1 [hep-th] 4 Jan 2023
|
| 22 |
+
|
| 23 |
+
Contents
|
| 24 |
+
1
|
| 25 |
+
Introduction
|
| 26 |
+
1
|
| 27 |
+
2
|
| 28 |
+
Inside holographic Weyl semimetal
|
| 29 |
+
3
|
| 30 |
+
2.1
|
| 31 |
+
Inner structures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
|
| 32 |
+
4
|
| 33 |
+
2.2
|
| 34 |
+
Behaviors of Kasner exponents . . . . . . . . . . . . . . . . . . . . . . . .
|
| 35 |
+
5
|
| 36 |
+
2.3
|
| 37 |
+
Proper time of timelike geodesics
|
| 38 |
+
. . . . . . . . . . . . . . . . . . . . . .
|
| 39 |
+
9
|
| 40 |
+
3
|
| 41 |
+
Inside holographic nodal line semimetal
|
| 42 |
+
10
|
| 43 |
+
3.1
|
| 44 |
+
Kasner exponents . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
|
| 45 |
+
12
|
| 46 |
+
3.2
|
| 47 |
+
Proper time of timelike geodesics
|
| 48 |
+
. . . . . . . . . . . . . . . . . . . . . .
|
| 49 |
+
15
|
| 50 |
+
4
|
| 51 |
+
Conclusion and discussion
|
| 52 |
+
15
|
| 53 |
+
A Equations in holographic WSM
|
| 54 |
+
16
|
| 55 |
+
B Equations in holographic NLSM
|
| 56 |
+
18
|
| 57 |
+
1
|
| 58 |
+
Introduction
|
| 59 |
+
The conventional classifications on the phases of matter are rooted in the Landau paradigm
|
| 60 |
+
of symmetry breaking theory [1]. Over the past thirty years, new states of matter have
|
| 61 |
+
been found which are beyond the concept of Landau paradigm.
|
| 62 |
+
One example is the
|
| 63 |
+
topological states of matter, including the quantum Hall states, topological insulators,
|
| 64 |
+
topological semimetals and so on [2]. Different from the conventional Landau paradigm,
|
| 65 |
+
there is no symmetry breaking during the topological phase transition and it attracts lots
|
| 66 |
+
of research attention.
|
| 67 |
+
In recent years, the strongly interacting topological Weyl semimetals (WSM) [3,4] and
|
| 68 |
+
nodal line semimetals (NLSM) [5,6] have been explicitly constructed from the holographic
|
| 69 |
+
duality. Both holographic WSM and NLSM are shown to possess nontrivial topological
|
| 70 |
+
invariants [7]. Remarkably, holographic WSM exhibits interesting effects inherited from
|
| 71 |
+
the boundary states [8]. These features suggest that the physical properties associated to
|
| 72 |
+
topology from the weakly coupled field theories persist in the strongly coupled topologi-
|
| 73 |
+
cal systems from the holography. Moreover, the systems could go through a topological
|
| 74 |
+
phase transition to a topologically trivial semimetal phase, see [9] for a review on the
|
| 75 |
+
1
|
| 76 |
+
|
| 77 |
+
developments.4
|
| 78 |
+
In the holographic WSM, during the topological phase transition the
|
| 79 |
+
anomalous Hall conductivity could be served as an order parameter, while in the holo-
|
| 80 |
+
graphic NLSM it is not clear about the order parameters. Whether possible universal
|
| 81 |
+
“order parameter” exist for the topological phase transitions? What is the topological
|
| 82 |
+
nature in the topological phase from holography? These are elusive problems we aim to
|
| 83 |
+
explore from the holographic duality.
|
| 84 |
+
In holography, the thermal states are dual to black hole geometries in the bulk. The
|
| 85 |
+
black hole interior is expected to encode important information of the dual field the-
|
| 86 |
+
ory [28–30]. In the case that the thermal states are described by the black holes with
|
| 87 |
+
simple Kasner singularities, it has been shown recently in [31] that the order of the ther-
|
| 88 |
+
mal phase transition in the dual field theory is connected to the behavior of the Kasner
|
| 89 |
+
exponents of the black hole singularity.5 For the topological phase transitions in holo-
|
| 90 |
+
graphic topological semimetals at finite temperature, the systems experience a smooth
|
| 91 |
+
crossover from a topological phase, a critical phase to a trivial phase. Although the phase
|
| 92 |
+
crossover is different from thermal phase transitions, it is still interesting to explore the
|
| 93 |
+
interior geometries in holographic topological semimetals, in order to uncover possible
|
| 94 |
+
universal behavior during the topological phase transitions.
|
| 95 |
+
It turns out that there exist both universal and special behaviors of the singularities
|
| 96 |
+
in holographic topological semimetals. The universal behavior is similar to the topolog-
|
| 97 |
+
ical nature of topological phase and might give hints to the problems we raised for the
|
| 98 |
+
topological semimetals, while the special features can be understood from the fact that
|
| 99 |
+
the holographic WSM and the holographic NLSM share similarities and also differences
|
| 100 |
+
in the constructions as emphasized in [5, 7]. More precisely, in both cases, two matters
|
| 101 |
+
fields are added which play same role from the point of view of the boundary field theory,
|
| 102 |
+
while they play different roles in the bulk geometry. In the boundary field theory, one of
|
| 103 |
+
the two matter fields is to deform the Dirac point into two Weyl nodes or a nodal line,
|
| 104 |
+
while the other matter field is to gap the system. In the bulk, in the topological phase
|
| 105 |
+
of holographic WSM the IR geometry of Schwarzschild black hole is not deformed by the
|
| 106 |
+
matter fields, while the backreaction of the matter fields on the gravitational geometry is
|
| 107 |
+
quite strong in IR in the topological phase of holographic NLSM. We will see that these
|
| 108 |
+
two different situations lead to different properties of the black hole singularities in the
|
| 109 |
+
topological phases.
|
| 110 |
+
It is known that the information of the interior geometry can be probed from the
|
| 111 |
+
geodesics which correspond to certain correlators in the dual field theory. For example,
|
| 112 |
+
the proper time from the horizon to the singularity can be extracted from the thermal
|
| 113 |
+
one point function of certain heavy operator [30]. We will compute this quantity in the
|
| 114 |
+
4Other interesting developments can be found in e.g. [10–27].
|
| 115 |
+
5Other studies on the geometric aspects of black hole singularities can be found in e.g. [32–53].
|
| 116 |
+
2
|
| 117 |
+
|
| 118 |
+
bulk and study its behavior in the topological phases and trivial phases.
|
| 119 |
+
This paper is organized as follows. In Sec. 2, we will first review the holographic WSM
|
| 120 |
+
and then study its interior geometry as well as the proper time of the timelike geodesics.
|
| 121 |
+
In Sec. 3, we will review the holographic NLSM and then also study its interior geometry
|
| 122 |
+
and the proper time of the timelike geodesics. Sec. 4 is devoted to the conclusions and
|
| 123 |
+
open questions. The details of calculations are in the appendices.
|
| 124 |
+
2
|
| 125 |
+
Inside holographic Weyl semimetal
|
| 126 |
+
In this section we first briefly review the holographic WSM which describes a topological
|
| 127 |
+
phase transition from topological WSM phase to a trivial semimetal phase. Then we
|
| 128 |
+
study the interior geometry of the black hole solutions and discuss the possible universal
|
| 129 |
+
behavior of the black hole singularities as well as the interior geometry. We also comment
|
| 130 |
+
on the possible observable as the role of “order parameter” during the topological phase
|
| 131 |
+
transition.
|
| 132 |
+
The action of the holographic WSM [3,4] is
|
| 133 |
+
S =
|
| 134 |
+
�
|
| 135 |
+
d5x√−g
|
| 136 |
+
� 1
|
| 137 |
+
2κ2
|
| 138 |
+
�
|
| 139 |
+
R + 12
|
| 140 |
+
L2
|
| 141 |
+
�
|
| 142 |
+
− 1
|
| 143 |
+
4F2 − 1
|
| 144 |
+
4F 2 + α
|
| 145 |
+
3 ϵabcdeAa
|
| 146 |
+
�
|
| 147 |
+
FbcFde + 3FbcFde
|
| 148 |
+
�
|
| 149 |
+
− (DaΦ)∗(DaΦ) − V (Φ)
|
| 150 |
+
�
|
| 151 |
+
,
|
| 152 |
+
(2.1)
|
| 153 |
+
where two gauge fields are dual to vector and axial currents respectively. A special Chern-
|
| 154 |
+
Simons structure is introduced to match the Wald identity for these currents. An axially
|
| 155 |
+
charged scalar field Φ is also introduced in the model with the source interpreted as the
|
| 156 |
+
mass term. Note that DaΦ = ∂aΦ − iqAaΦ where Aa is the axial U(1) gauge potential,
|
| 157 |
+
and V (Φ) = m2|Φ|2 + λ
|
| 158 |
+
2|Φ|4. We set 2κ2 = L = 1.
|
| 159 |
+
We focus on the finite temperature and use the following ansatz
|
| 160 |
+
ds2 = −udt2 + dr2
|
| 161 |
+
u + f(dx2 + dy2) + hdz2 ,
|
| 162 |
+
A = Azdz ,
|
| 163 |
+
Φ = φ .
|
| 164 |
+
(2.2)
|
| 165 |
+
The equations of motion for the fields can be found in the appendix A. In the following we
|
| 166 |
+
consider m2 = −3, q = 1, λ = 1/10. Generalization to the other values of the parameters
|
| 167 |
+
is straightforward.
|
| 168 |
+
We use the following boundary conditions for the matter fields
|
| 169 |
+
lim
|
| 170 |
+
r→∞ Az = b ,
|
| 171 |
+
lim
|
| 172 |
+
r→∞ rφ = M ,
|
| 173 |
+
(2.3)
|
| 174 |
+
3
|
| 175 |
+
|
| 176 |
+
where b is the time reversal symmetry breaking parameter which play the role of split-
|
| 177 |
+
ting a Dirac point into two Weyl points, and M is the mass parameter which gaps the
|
| 178 |
+
Dirac point. The competing between these two effects leads to interesting topological
|
| 179 |
+
phase transitions. The system is completely determined by the dimensionless parameters
|
| 180 |
+
T/b, M/b.
|
| 181 |
+
In the weakly coupled WSM, the quantum topological phase transition could be man-
|
| 182 |
+
ifest from both the band structure and equivalently the behavior of the anomalous Hall
|
| 183 |
+
conductivity. In the strongly coupled model from holography, the anomalous Hall con-
|
| 184 |
+
ductivity behaves similarly to the weakly coupled case, indicating that there is a topo-
|
| 185 |
+
logical phase transition, as shown in Fig. 1. The lines in red, blue and purple are for
|
| 186 |
+
T/b = 0.05, 0.02, 0.01 respectively. The transition becomes sharp at zero temperature
|
| 187 |
+
and the dashed gray line is the critical value of the transition at zero temperature.
|
| 188 |
+
���
|
| 189 |
+
���
|
| 190 |
+
���
|
| 191 |
+
���
|
| 192 |
+
���
|
| 193 |
+
���
|
| 194 |
+
���
|
| 195 |
+
���
|
| 196 |
+
���
|
| 197 |
+
���
|
| 198 |
+
���
|
| 199 |
+
���
|
| 200 |
+
���
|
| 201 |
+
M
|
| 202 |
+
b
|
| 203 |
+
σAHE
|
| 204 |
+
8 α b
|
| 205 |
+
Figure 1:
|
| 206 |
+
Plot of anomalous Hall conductivity as a function of M/b at the temperatures
|
| 207 |
+
T/b = 0.05 (red), 0.02 (blue), 0.01 (purple). The gray dashed line is the critical value of M/b
|
| 208 |
+
of the quantum phase transition at zero temperature.
|
| 209 |
+
2.1
|
| 210 |
+
Inner structures
|
| 211 |
+
The phase transitions could be parameterized by the anomalous Hall conductivity which
|
| 212 |
+
is completely determined by the horizon value of the axial gauge field Az. Given the
|
| 213 |
+
possible connection between the physics inside and outside the horizon, it is interesting
|
| 214 |
+
to study the black hole inner structures during the topological phase transitions.
|
| 215 |
+
From the black hole solutions we have obtained, we could integrate the system further
|
| 216 |
+
to the singularity since the geometry is smooth at the horizon. We find that at low
|
| 217 |
+
temperature, the matter field φ oscillates inside the horizon only in the topological phase
|
| 218 |
+
4
|
| 219 |
+
|
| 220 |
+
(i.e. M/b < 0.744). The typical behavior is shown in Fig. 2, where the oscillation regime
|
| 221 |
+
of the scalar field φ (which has been rescaled according to φ/φh) as a function of r/rh
|
| 222 |
+
at fixed T/b (left) or M/b (right) are plotted respectively. We find that when we fix
|
| 223 |
+
the temperature T/b, the times of oscilation become less when we increase M/b from 0
|
| 224 |
+
to (M/b)c. Furthermore, when we fix M/b < (M/b)c, the lower temperature, the more
|
| 225 |
+
times that φ oscillates. Note that the other fields do not show any oscillation from the
|
| 226 |
+
horizon to the singularity.
|
| 227 |
+
Different from the holographic superconductor cases, the oscillation here is not related
|
| 228 |
+
to the collapse of Einstein-Rosen bridge [34], since there is no inner horizon any more
|
| 229 |
+
for holographic WSM. Similar oscillation behavior has been found previously in neutral
|
| 230 |
+
helical black holes [35].
|
| 231 |
+
���
|
| 232 |
+
���
|
| 233 |
+
���
|
| 234 |
+
���
|
| 235 |
+
���
|
| 236 |
+
���
|
| 237 |
+
-���
|
| 238 |
+
-���
|
| 239 |
+
-���
|
| 240 |
+
���
|
| 241 |
+
���
|
| 242 |
+
���
|
| 243 |
+
r
|
| 244 |
+
rh
|
| 245 |
+
ϕ
|
| 246 |
+
ϕh
|
| 247 |
+
���
|
| 248 |
+
���
|
| 249 |
+
���
|
| 250 |
+
���
|
| 251 |
+
���
|
| 252 |
+
���
|
| 253 |
+
-���
|
| 254 |
+
-���
|
| 255 |
+
���
|
| 256 |
+
���
|
| 257 |
+
���
|
| 258 |
+
r
|
| 259 |
+
rh
|
| 260 |
+
ϕ
|
| 261 |
+
ϕh
|
| 262 |
+
Figure 2: The plots of φ/φh along radial direction in the oscillation region at fixed T/b = 0.02
|
| 263 |
+
(left) while M/b = 0.1 (purple), 0.4 (blue), 0.6 (orange), 0.74 (red), as well as at fixed M/b = 0.1
|
| 264 |
+
(right) while T/b = 0.05 (red), 0.02 (blue), 0.01 (purple). Here φh is the horizon value of φ.
|
| 265 |
+
2.2
|
| 266 |
+
Behaviors of Kasner exponents
|
| 267 |
+
The interior solution can be further integrated to the singularity. Near the singularity
|
| 268 |
+
rs, we assume that at the leading order the fields behave as
|
| 269 |
+
u ∼ −u0(r − rs)nu ,
|
| 270 |
+
f ∼ f0(r − rs)nf ,
|
| 271 |
+
h ∼ h0(r − rs)nh ,
|
| 272 |
+
φ ∼ nφ ln(r − rs) , (2.4)
|
| 273 |
+
where u0, f0, h0 and nu, nf, nh, nφ are all constants. Here u0, f0, h0 depend on the scaling
|
| 274 |
+
symmetry in (A.3),(A.4),(A.5) while nu, nf, nh, nφ are not. Also note that here rs is not
|
| 275 |
+
necessarily to be zero since there is a shift symmetry of the system r → r + α along the
|
| 276 |
+
radial direction which was used to set the boundary behavior (A.8). Moreover, as we
|
| 277 |
+
shall see later, the axial gauge field Az is determined by the ansatz (2.4).
|
| 278 |
+
5
|
| 279 |
+
|
| 280 |
+
Near the singularity the equations of motion (A.6) can be simplified under the assump-
|
| 281 |
+
tion that the ignored terms are subleading which will be numerically checked afterward,
|
| 282 |
+
u′′ + h′
|
| 283 |
+
2hu′ −
|
| 284 |
+
�
|
| 285 |
+
f ′′ + f ′h′
|
| 286 |
+
2h
|
| 287 |
+
� u
|
| 288 |
+
f = 0 ,
|
| 289 |
+
f ′′
|
| 290 |
+
f + u′′
|
| 291 |
+
2u − f ′2
|
| 292 |
+
4f 2 + f ′u′
|
| 293 |
+
fu + 1
|
| 294 |
+
2φ′2 = 0 ,
|
| 295 |
+
1
|
| 296 |
+
2φ′2 − u′
|
| 297 |
+
2u
|
| 298 |
+
�f ′
|
| 299 |
+
f + h′
|
| 300 |
+
2h
|
| 301 |
+
�
|
| 302 |
+
− f ′h′
|
| 303 |
+
2fh − f ′2
|
| 304 |
+
4f 2 = 0 ,
|
| 305 |
+
A′′
|
| 306 |
+
z +
|
| 307 |
+
�f ′
|
| 308 |
+
f − h′
|
| 309 |
+
2h + u′
|
| 310 |
+
u
|
| 311 |
+
�
|
| 312 |
+
A′
|
| 313 |
+
z = 0 ,
|
| 314 |
+
φ′′ +
|
| 315 |
+
�f ′
|
| 316 |
+
f + h′
|
| 317 |
+
2h + u′
|
| 318 |
+
u
|
| 319 |
+
�
|
| 320 |
+
φ′ = 0 .
|
| 321 |
+
(2.5)
|
| 322 |
+
Substituting (2.4) into (2.5), we obtain
|
| 323 |
+
nh = 2 (1 − nu − nf) ,
|
| 324 |
+
nφ = ±
|
| 325 |
+
�
|
| 326 |
+
(2nf + nu)(1 − nu) − 3n2
|
| 327 |
+
f
|
| 328 |
+
2 .
|
| 329 |
+
(2.6)
|
| 330 |
+
We can also solve the fourth equation in (2.5) to obtain at leading order Az
|
| 331 |
+
Az ≃ Azs0 + Azs1(r − rs)nh .
|
| 332 |
+
(2.7)
|
| 333 |
+
Note that the leading term Azs0 can be rescaled to be 1, while Azs1 could be determined
|
| 334 |
+
from the radial conserved quantities as will be discussed later. Thus there are only two
|
| 335 |
+
independent parameters in (2.4) and (2.7).
|
| 336 |
+
Note that in the above equations (2.5), we have assumed that the terms ignored are
|
| 337 |
+
subleading. More explicitly, we have assumed
|
| 338 |
+
nu < 2 ,
|
| 339 |
+
nf + nu < 1 ,
|
| 340 |
+
2nf + nu > 0 .
|
| 341 |
+
(2.8)
|
| 342 |
+
Numerically we have checked that all the above relations are satisfied for the parameters
|
| 343 |
+
we have considered, which indicates that the singularities are stable and of form (2.4)
|
| 344 |
+
and (2.7).
|
| 345 |
+
There are two radical conserved charge associated to the scaling symmetries of the
|
| 346 |
+
system,
|
| 347 |
+
Q1 =
|
| 348 |
+
√
|
| 349 |
+
h(u′f − uf ′) ,
|
| 350 |
+
(2.9)
|
| 351 |
+
Q2 = u′√
|
| 352 |
+
hf − h′
|
| 353 |
+
√
|
| 354 |
+
h
|
| 355 |
+
uf − AzA′
|
| 356 |
+
z
|
| 357 |
+
uf
|
| 358 |
+
√
|
| 359 |
+
h
|
| 360 |
+
.
|
| 361 |
+
(2.10)
|
| 362 |
+
6
|
| 363 |
+
|
| 364 |
+
We have used them to check the accuracy of the numerics. Moreover, evaluate them at
|
| 365 |
+
the horizon and at the singularity we obtain
|
| 366 |
+
4πTf1
|
| 367 |
+
�
|
| 368 |
+
h1 = Ts = u0f0
|
| 369 |
+
�
|
| 370 |
+
h0(nf − nu)
|
| 371 |
+
(2.11)
|
| 372 |
+
= u0f0
|
| 373 |
+
√h0
|
| 374 |
+
(nhAzs0Azs1 − h0(2nf + 3nu − 2) )
|
| 375 |
+
(2.12)
|
| 376 |
+
where s is the density of entropy. From (2.11), we have nf > nu in addition to the con-
|
| 377 |
+
straints (2.8). Moreover, the above two conserved quantities give the relations nhAzs0Azs1 =
|
| 378 |
+
h0(3nf +2nu −2) which turns out to be zero in the topological phase at low temperature
|
| 379 |
+
where Azs1 = 3nf + 2nu − 2 = 0.
|
| 380 |
+
Starting from (2.2, 2.4) and performing the coordinate transformation
|
| 381 |
+
τ = −
|
| 382 |
+
2
|
| 383 |
+
√n0(nu − 2)(r − rs)(2−nu)/2 ,
|
| 384 |
+
(2.13)
|
| 385 |
+
we obtain the Kasner form for the fields
|
| 386 |
+
ds2 = −dτ 2 + ctτ 2ptdt2 + cxτ 2px(dx2 + dy2) + czτ 2pzdz2 ,
|
| 387 |
+
φ = pφ log τ + cφ ,
|
| 388 |
+
(2.14)
|
| 389 |
+
where
|
| 390 |
+
pt =
|
| 391 |
+
nu
|
| 392 |
+
2 − nu
|
| 393 |
+
,
|
| 394 |
+
px =
|
| 395 |
+
nf
|
| 396 |
+
2 − nu
|
| 397 |
+
,
|
| 398 |
+
pz =
|
| 399 |
+
nh
|
| 400 |
+
2 − nu
|
| 401 |
+
,
|
| 402 |
+
pφ =
|
| 403 |
+
2nφ
|
| 404 |
+
2 − nu
|
| 405 |
+
.
|
| 406 |
+
(2.15)
|
| 407 |
+
Note that Az is a constant at the leading order. Using the relations (2.6), the above
|
| 408 |
+
Kasner exponents can be expressed in terms of nu and nf,
|
| 409 |
+
pt =
|
| 410 |
+
nu
|
| 411 |
+
2 − nu
|
| 412 |
+
,
|
| 413 |
+
px =
|
| 414 |
+
nf
|
| 415 |
+
2 − nu
|
| 416 |
+
,
|
| 417 |
+
pz = 2(1 − nu − nf)
|
| 418 |
+
2 − nu
|
| 419 |
+
,
|
| 420 |
+
pφ = ±
|
| 421 |
+
�
|
| 422 |
+
4(2nf + nu)(1 − nu) − 6n2
|
| 423 |
+
f
|
| 424 |
+
2 − nu
|
| 425 |
+
.
|
| 426 |
+
(2.16)
|
| 427 |
+
Note that the sign of pφ in (2.16) can only be determined from numerics. They satisfy
|
| 428 |
+
the following Kasner relations
|
| 429 |
+
pt + 2px + pz = 1 ,
|
| 430 |
+
p2
|
| 431 |
+
t + 2p2
|
| 432 |
+
x + p2
|
| 433 |
+
z + p2
|
| 434 |
+
φ = 1 .
|
| 435 |
+
(2.17)
|
| 436 |
+
It indicates that only two of the four Kasner exponents are independent.
|
| 437 |
+
In Fig. 3, we show the Kasner exponents as a function of M/b at different tempera-
|
| 438 |
+
tures T/b = 0.05 (red), 0.02 (blue), 0.01 (purple). We find that at low temperature, the
|
| 439 |
+
Kasner exponents in the Weyl semimetal phase take the same value of the Schwarzschild
|
| 440 |
+
black hole (e.g. within the difference of order less than 10−9 between M/b = 0.5 and
|
| 441 |
+
M/b = 0 at T/b = 0.01). This reminds us the topological feature in terms of the black
|
| 442 |
+
7
|
| 443 |
+
|
| 444 |
+
hole singularity. It is related to the fact that the matter fields do not backreact relevantly
|
| 445 |
+
to the Schwarzschild solution in the topological phase, i.e. the probe limit of system in
|
| 446 |
+
terms of matter fields in the Schwarzschild black hole background works well. We have
|
| 447 |
+
also checked that inside the black holes, in the topological phase the matter fields ob-
|
| 448 |
+
tained from the backreacted case match well with the solutions obtained from the probe
|
| 449 |
+
limit. In the quantum critical regime, the Kasner exponents oscillate. While in the trivial
|
| 450 |
+
phase, the Kasner exponent does not have any oscillate behavior.
|
| 451 |
+
���
|
| 452 |
+
���
|
| 453 |
+
���
|
| 454 |
+
���
|
| 455 |
+
���
|
| 456 |
+
���
|
| 457 |
+
���
|
| 458 |
+
-����
|
| 459 |
+
-����
|
| 460 |
+
-����
|
| 461 |
+
-����
|
| 462 |
+
-����
|
| 463 |
+
-����
|
| 464 |
+
M
|
| 465 |
+
b
|
| 466 |
+
pt
|
| 467 |
+
���
|
| 468 |
+
���
|
| 469 |
+
���
|
| 470 |
+
���
|
| 471 |
+
���
|
| 472 |
+
���
|
| 473 |
+
���
|
| 474 |
+
-���
|
| 475 |
+
-���
|
| 476 |
+
-���
|
| 477 |
+
���
|
| 478 |
+
���
|
| 479 |
+
���
|
| 480 |
+
M
|
| 481 |
+
b
|
| 482 |
+
pϕ
|
| 483 |
+
���
|
| 484 |
+
���
|
| 485 |
+
���
|
| 486 |
+
���
|
| 487 |
+
���
|
| 488 |
+
���
|
| 489 |
+
���
|
| 490 |
+
����
|
| 491 |
+
����
|
| 492 |
+
����
|
| 493 |
+
����
|
| 494 |
+
����
|
| 495 |
+
����
|
| 496 |
+
M
|
| 497 |
+
b
|
| 498 |
+
px
|
| 499 |
+
���
|
| 500 |
+
���
|
| 501 |
+
���
|
| 502 |
+
���
|
| 503 |
+
���
|
| 504 |
+
���
|
| 505 |
+
���
|
| 506 |
+
����
|
| 507 |
+
����
|
| 508 |
+
����
|
| 509 |
+
����
|
| 510 |
+
M
|
| 511 |
+
b
|
| 512 |
+
pz
|
| 513 |
+
Figure 3: Plots of Kasner exponents as a function of M/b. For all cases we have T/b = 0.05
|
| 514 |
+
(red), 0.02 (blue), 0.01 (purple). The dashed gray vertical lines are the Kasner exponents of
|
| 515 |
+
five dimension Schwarzschild black hole.
|
| 516 |
+
Note that in [5], a paradigm for constructing the topological phase was proposed
|
| 517 |
+
and the holographic Weyl semimetal belongs to the first type, where the matter fields are
|
| 518 |
+
irrelevant in the IR of the Schwarzschild black hole. It seems likely that in any topological
|
| 519 |
+
phase of this kind, the singularities are of Kasner form taking values of Schwarzschild
|
| 520 |
+
black hole.
|
| 521 |
+
8
|
| 522 |
+
|
| 523 |
+
2.3
|
| 524 |
+
Proper time of timelike geodesics
|
| 525 |
+
One of interesting connection between the interior geometry and the boundary observable
|
| 526 |
+
is given in [30] that the proper time of radial timelike geodesic can be encoded in the
|
| 527 |
+
thermal one point functions of heavy operators. It is thus interesting to study the proper
|
| 528 |
+
time of radial timelike geodesics to see if it has specific behavior during the topological
|
| 529 |
+
phase transitions.
|
| 530 |
+
We consider radial timelike geodesic for which gtt ˙t2 + grr ˙r2 = −1, where the dot
|
| 531 |
+
denotes the derivative with respect to the proper time τ. Along the geodesic there is a
|
| 532 |
+
conserved charge E = −gtt ˙t which can be interpreted as energy. Then the equation of
|
| 533 |
+
motion of the geodesic becomes
|
| 534 |
+
E2
|
| 535 |
+
gtt
|
| 536 |
+
+ grr ˙r2 = −1 ,
|
| 537 |
+
(2.18)
|
| 538 |
+
from which we obtain
|
| 539 |
+
dτ
|
| 540 |
+
dr =
|
| 541 |
+
1
|
| 542 |
+
√
|
| 543 |
+
E2 − u .
|
| 544 |
+
(2.19)
|
| 545 |
+
The proper time from the horizon to the singularity of a particle with E = 0 (i.e. the
|
| 546 |
+
longest time) is
|
| 547 |
+
τs =
|
| 548 |
+
� rh
|
| 549 |
+
rs
|
| 550 |
+
dr
|
| 551 |
+
√−u .
|
| 552 |
+
(2.20)
|
| 553 |
+
The plots of τs as a function of M/b for different T/b are shown in Fig. 4.
|
| 554 |
+
���
|
| 555 |
+
���
|
| 556 |
+
���
|
| 557 |
+
���
|
| 558 |
+
���
|
| 559 |
+
���
|
| 560 |
+
���
|
| 561 |
+
���
|
| 562 |
+
���
|
| 563 |
+
���
|
| 564 |
+
���
|
| 565 |
+
���
|
| 566 |
+
M
|
| 567 |
+
b
|
| 568 |
+
τs
|
| 569 |
+
Figure 4: Plots of the proper time τs from the horizon to the singularity as a function of M/b
|
| 570 |
+
at different temperatures T/b = 0.05 (red), 0.02 (blue), 0.01 (purple).
|
| 571 |
+
The proper time from the horizon to the singularity in the topological phase is equal
|
| 572 |
+
to the case of Schwarzschild black hole τs = π/4 (e.g. within the difference of order less
|
| 573 |
+
9
|
| 574 |
+
|
| 575 |
+
than 10−4 between M/b = 0.5 and M/b = 0 at T/b = 0.01). This is expected from
|
| 576 |
+
the fact that in the topological phase at low temperature the interior of the black holes
|
| 577 |
+
match well with the Schwarzschild black hole. In the topologically trivial phase τs is
|
| 578 |
+
monotonically decreasing. Moreover, τs shows a jump behavior and takes a maximum
|
| 579 |
+
value in the critical regime. Note that τs is encoded in the thermal one point function
|
| 580 |
+
of heavy operators in the form of ⟨O⟩ ∝ e−imτs where the complexified mass m has
|
| 581 |
+
Im(m) < 0 [30]. One might use this thermal one point function as the “order” parameter
|
| 582 |
+
for the topological phase transition. The behavior of the proper time also reminds us the
|
| 583 |
+
behavior of the dimensionless information screening length in [14]. One obvious difference
|
| 584 |
+
is that the information screening length is determined by the quantities at the horizon,
|
| 585 |
+
while τs is determined by the geometry from the horizon to the singularity.
|
| 586 |
+
3
|
| 587 |
+
Inside holographic nodal line semimetal
|
| 588 |
+
In the previous section, we have seen that the interior of the black hole geometries
|
| 589 |
+
for the holographic WSM exhibit interesting behavior. In the topological WSM phase,
|
| 590 |
+
the Kasner exponents of the dual geometries take the same value of the Schwarzschild
|
| 591 |
+
black hole at low temperature, as shown in Fig. 3. Moreover, the dual operator which
|
| 592 |
+
encodes the proper time from the horizon to the singularity could be served as an “order
|
| 593 |
+
parameter” during the topological phase transition, as shown in Fig. 4. To check if these
|
| 594 |
+
behaviors are universal for any topological phase transitions, in this section we study the
|
| 595 |
+
other topological phase transition model from holography, i.e. the holographic NLSM
|
| 596 |
+
model which describes a phase transition from the topological NLSM phase to a trivial
|
| 597 |
+
semimetal phase [5,6].
|
| 598 |
+
The action for the holographic NLSM [6] is
|
| 599 |
+
S =
|
| 600 |
+
�
|
| 601 |
+
d5x √−g
|
| 602 |
+
� 1
|
| 603 |
+
2κ2
|
| 604 |
+
�
|
| 605 |
+
R + 12
|
| 606 |
+
L2
|
| 607 |
+
�
|
| 608 |
+
− 1
|
| 609 |
+
4F2 − 1
|
| 610 |
+
4F 2 + α
|
| 611 |
+
3 ϵabcdeAa
|
| 612 |
+
�
|
| 613 |
+
FbcFde + 3FbcFde
|
| 614 |
+
�
|
| 615 |
+
− (DaΦ)∗(DaΦ) − V1(Φ) − 1
|
| 616 |
+
6ηϵabcde�
|
| 617 |
+
iBabH∗
|
| 618 |
+
cde − iB∗
|
| 619 |
+
abHcde
|
| 620 |
+
�
|
| 621 |
+
− V2(Bab) − λ|Φ|2B∗
|
| 622 |
+
abBab
|
| 623 |
+
�
|
| 624 |
+
,
|
| 625 |
+
(3.1)
|
| 626 |
+
where Fab = ∂aVb − ∂bVa is the vector gauge field strength. Fab = ∂aAb − ∂bAa is the
|
| 627 |
+
axial gauge field strength. Da = ∇a −iq1Aa is the covariant derivative and q1 is the axial
|
| 628 |
+
charge of scalar field. α is the Chern-Simons coupling. Bab is an antisymmetric complex
|
| 629 |
+
two form field with the field strength
|
| 630 |
+
Habc = ∂aBbc + ∂bBca + ∂cBab − iq2AaBbc − iq2AbBca − iq2AcBab ,
|
| 631 |
+
(3.2)
|
| 632 |
+
10
|
| 633 |
+
|
| 634 |
+
where q2 is the axial charge of the two form field. η is the Chern-Simons coupling strength
|
| 635 |
+
of the two form field. The introduction of the Chern-Simons terms while not canonical
|
| 636 |
+
kinetic term for the two form field follows from the self-duality condition of the two form
|
| 637 |
+
operator in the weakly coupled theory [6]. The potential terms are chosen as
|
| 638 |
+
V1 = m2
|
| 639 |
+
1|Φ|2 + λ1
|
| 640 |
+
2 |Φ|4 ,
|
| 641 |
+
V2 = m2
|
| 642 |
+
2B∗
|
| 643 |
+
abBab ,
|
| 644 |
+
(3.3)
|
| 645 |
+
where m2
|
| 646 |
+
1 and m2
|
| 647 |
+
2 are the mass parameters of the scalar field and the two form field. The
|
| 648 |
+
λ term in the action (3.1) denotes the interaction between the scalar field and the two
|
| 649 |
+
form field. We set 2κ2 = L = 1.
|
| 650 |
+
Similar to the holographic WSM, we focus on the finite temperature solution and take
|
| 651 |
+
the ansatz
|
| 652 |
+
ds2 = −udt2 + dr2
|
| 653 |
+
u + f(dx2 + dy2) + hdz2 ,
|
| 654 |
+
Φ = φ ,
|
| 655 |
+
Bxy = −Byx = Bxy ,
|
| 656 |
+
Btz = −Bzt = iBtz .
|
| 657 |
+
(3.4)
|
| 658 |
+
Plugging the above ansatz into the equations of motion, we could obtain the dynamical
|
| 659 |
+
equations of the fields, which can be found in the appendix B. In the following we choose
|
| 660 |
+
m2
|
| 661 |
+
1 = −3, m2
|
| 662 |
+
2 = 1, η = 2 and q1 = q2 = 1, λ = 1, λ1 = 0.1 for simplicity.
|
| 663 |
+
With the following boundary conditions,
|
| 664 |
+
lim
|
| 665 |
+
r→∞ rφ = M ,
|
| 666 |
+
lim
|
| 667 |
+
r→∞
|
| 668 |
+
Bxy
|
| 669 |
+
r
|
| 670 |
+
= lim
|
| 671 |
+
r→∞
|
| 672 |
+
Btz
|
| 673 |
+
r
|
| 674 |
+
= b ,
|
| 675 |
+
(3.5)
|
| 676 |
+
we can integrate the system from the boundary to the horizon. Different from the holo-
|
| 677 |
+
graphic WSM, in holographic NLSM there is no sharp “order parameter” like anomalous
|
| 678 |
+
Hall conductivity. Nevertheless, it was found in [6] that at zero temperature, the dual
|
| 679 |
+
fermionic spectral function shows multiple Fermi surfaces with the topology of nodal lines
|
| 680 |
+
when M/b < (M/b)c while it is gapped when M/b > (M/b)c. This indicates that the
|
| 681 |
+
system undergoes a topological phase transitions from topological NLSM to topologically
|
| 682 |
+
trivial semimetal phase.
|
| 683 |
+
With the regularity condition near the horizon, the system can be further integrated
|
| 684 |
+
to the singularity. In the following we will discuss the interior geometries and singularities
|
| 685 |
+
of the system.
|
| 686 |
+
11
|
| 687 |
+
|
| 688 |
+
3.1
|
| 689 |
+
Kasner exponents
|
| 690 |
+
Close to the singularity r → rs, similar to the holographic WSM case we again take the
|
| 691 |
+
ansatz
|
| 692 |
+
u ∼ −u0(r − rs)nu ,
|
| 693 |
+
f ∼ f0(r − rs)nf ,
|
| 694 |
+
h ∼ h0(r − rs)nh ,
|
| 695 |
+
φ ∼ nφ ln(r − rs) , (3.6)
|
| 696 |
+
where u0, f0, h0 and nu, nf, nh, nφ are all constants. The other two matter fields Btz and
|
| 697 |
+
Bxy will be determined by the above ansatz.
|
| 698 |
+
The equations of motion can be simplified close to the singularity under the assump-
|
| 699 |
+
tion that the ignored terms are subleading
|
| 700 |
+
u′′
|
| 701 |
+
u − f ′′
|
| 702 |
+
f + h′
|
| 703 |
+
2h
|
| 704 |
+
�u′
|
| 705 |
+
u − f ′
|
| 706 |
+
f
|
| 707 |
+
�
|
| 708 |
+
= 0 ,
|
| 709 |
+
u′′
|
| 710 |
+
2u + f ′′
|
| 711 |
+
f − f ′2
|
| 712 |
+
4f 2 + f ′u′
|
| 713 |
+
fu + 1
|
| 714 |
+
2φ′2 = 0 ,
|
| 715 |
+
f ′2
|
| 716 |
+
4f 2 + f ′h′
|
| 717 |
+
2fh + u′
|
| 718 |
+
2u
|
| 719 |
+
�f ′
|
| 720 |
+
f + h′
|
| 721 |
+
2h
|
| 722 |
+
�
|
| 723 |
+
− 1
|
| 724 |
+
2φ′2 = 0 ,
|
| 725 |
+
φ′′ +
|
| 726 |
+
�f ′
|
| 727 |
+
f + h′
|
| 728 |
+
2h + u′
|
| 729 |
+
u
|
| 730 |
+
�
|
| 731 |
+
φ′ = 0 ,
|
| 732 |
+
B′
|
| 733 |
+
tz − η
|
| 734 |
+
√
|
| 735 |
+
h
|
| 736 |
+
2f (λφ2)Bxy = 0 ,
|
| 737 |
+
B′
|
| 738 |
+
xy −
|
| 739 |
+
ηf
|
| 740 |
+
2
|
| 741 |
+
√
|
| 742 |
+
hu
|
| 743 |
+
(λφ2)Btz = 0 .
|
| 744 |
+
(3.7)
|
| 745 |
+
The first four equations in (3.7) are the same as the ones in holographic WSM. Similarly,
|
| 746 |
+
we obtain
|
| 747 |
+
nh = 2 (1 − nu − nf) ,
|
| 748 |
+
nφ = ±
|
| 749 |
+
�
|
| 750 |
+
(2nf + nu)(1 − nu) − 3n2
|
| 751 |
+
f
|
| 752 |
+
2 .
|
| 753 |
+
(3.8)
|
| 754 |
+
From the last two equations in (3.7) we have the following leading order solutions for the
|
| 755 |
+
two form fields near the singularity
|
| 756 |
+
Bxy ∼ Bxy0 + . . . ,
|
| 757 |
+
Btz ∼ Btz0 + . . . ,
|
| 758 |
+
(3.9)
|
| 759 |
+
where the dots are subleading terms of form (r − rs)2−nu−2nf(log(r − rs))2 and (r −
|
| 760 |
+
rs)2nf(log(r − rs))2 respectively. Here we have assumed 2 − nu − 2nf > 0 and nf > 0,
|
| 761 |
+
otherwise the leading solution of the two form field might be divergent. Similar to the
|
| 762 |
+
holographic WSM, these constants of the two form field depend on the scaling symmetry
|
| 763 |
+
of the system.
|
| 764 |
+
12
|
| 765 |
+
|
| 766 |
+
Note that in (3.7) we have assumed that the ignored terms are subleading. More
|
| 767 |
+
explicitly, we have assumed
|
| 768 |
+
nu < 2 ,
|
| 769 |
+
2nu + nh < 2 ,
|
| 770 |
+
nu + 2nf < 2 .
|
| 771 |
+
(3.10)
|
| 772 |
+
Note that the last two inequalities of above are consistent with the assumptions used in
|
| 773 |
+
obtaining (3.9). We have checked numerically that the inequalities (3.10) are satisfied for
|
| 774 |
+
the parameters we have considered.
|
| 775 |
+
Similar to the discussion in section 2.2, we can make a coordinate transformation
|
| 776 |
+
(2.13) to write the metric (3.6) into the Kasner form as (2.14) with the parameters (2.16)
|
| 777 |
+
and the Kasner relations (2.17). Here the leading order of the two form fields are constant
|
| 778 |
+
close to the singularity.
|
| 779 |
+
The two conserved charges of the scaling symmetries are
|
| 780 |
+
Q1 = 8
|
| 781 |
+
ηBtzBxy + u
|
| 782 |
+
√
|
| 783 |
+
h
|
| 784 |
+
(f ′h − fh′) ,
|
| 785 |
+
(3.11)
|
| 786 |
+
Q2 =
|
| 787 |
+
f
|
| 788 |
+
√
|
| 789 |
+
h
|
| 790 |
+
(u′h − uh′) .
|
| 791 |
+
(3.12)
|
| 792 |
+
Evaluate them at the horizon and at the singularity we obtain
|
| 793 |
+
8
|
| 794 |
+
ηBxy0Btz0 = u0f0
|
| 795 |
+
�
|
| 796 |
+
h0(nf − nh)
|
| 797 |
+
(3.13)
|
| 798 |
+
and
|
| 799 |
+
4πTf1
|
| 800 |
+
�
|
| 801 |
+
h1 = Ts = u0f0
|
| 802 |
+
�
|
| 803 |
+
h0(2 − 2nf − 3nu)
|
| 804 |
+
(3.14)
|
| 805 |
+
where s is the density of entropy. We have checked the above relations numerically.
|
| 806 |
+
In Fig. 5, we show the Kasner exponents for the holographic NLSM as functions of
|
| 807 |
+
M/b at different temperature T/b = 0.05 (red), 0.02 (blue), 0.01 (purple). We find that
|
| 808 |
+
at low temperature, the Kasner exponents pt, px, pz of the metric fields in the NLSM
|
| 809 |
+
semimetal phase are almost constant in the topological phase (e.g. within the difference
|
| 810 |
+
of order less than 1% between M/b = 0.5 and M/b = 0 at T/b = 0.01), which is quite
|
| 811 |
+
similar to the holographic WSM, while pφ changes a lot in the topological phase. Note
|
| 812 |
+
that this is consistent with the Kasner relations (2.17) since pφ is small. It is expected that
|
| 813 |
+
at extremely low temperature, the properties of the Kasner exponents in the holographic
|
| 814 |
+
NLSM might be the same as those in the holographic WSM, i.e. all the Kasner exponents
|
| 815 |
+
are constant. Due to numerical difficulty we have not explored such a low temperature
|
| 816 |
+
regime.
|
| 817 |
+
Different from the holographic WSM where the geometry is the same as Schwarzschild
|
| 818 |
+
black hole with a constant nonzero Az when M/b = 0. Here when M/b = 0, in the
|
| 819 |
+
13
|
| 820 |
+
|
| 821 |
+
���
|
| 822 |
+
���
|
| 823 |
+
���
|
| 824 |
+
���
|
| 825 |
+
���
|
| 826 |
+
-����
|
| 827 |
+
-����
|
| 828 |
+
-����
|
| 829 |
+
-����
|
| 830 |
+
-����
|
| 831 |
+
M
|
| 832 |
+
b
|
| 833 |
+
pt
|
| 834 |
+
���
|
| 835 |
+
���
|
| 836 |
+
���
|
| 837 |
+
���
|
| 838 |
+
���
|
| 839 |
+
-���
|
| 840 |
+
-���
|
| 841 |
+
-���
|
| 842 |
+
���
|
| 843 |
+
���
|
| 844 |
+
���
|
| 845 |
+
M
|
| 846 |
+
b
|
| 847 |
+
pϕ
|
| 848 |
+
���
|
| 849 |
+
���
|
| 850 |
+
���
|
| 851 |
+
���
|
| 852 |
+
���
|
| 853 |
+
����
|
| 854 |
+
����
|
| 855 |
+
����
|
| 856 |
+
����
|
| 857 |
+
����
|
| 858 |
+
����
|
| 859 |
+
����
|
| 860 |
+
M
|
| 861 |
+
b
|
| 862 |
+
px
|
| 863 |
+
���
|
| 864 |
+
���
|
| 865 |
+
���
|
| 866 |
+
���
|
| 867 |
+
���
|
| 868 |
+
���
|
| 869 |
+
���
|
| 870 |
+
���
|
| 871 |
+
���
|
| 872 |
+
���
|
| 873 |
+
M
|
| 874 |
+
b
|
| 875 |
+
pz
|
| 876 |
+
Figure 5: Plots of Kasner exponents for holographic NLSM as a function of M/b. For all cases
|
| 877 |
+
we have T/b = 0.05 (red), 0.02 (blue), 0.01 (purple). The horizontal dashed gray lines represent
|
| 878 |
+
the Kasner exponents for M/b = 0 at T/b = 0.01. The vertical dashed gray lines represent the
|
| 879 |
+
quantum critical point at zero temperature.
|
| 880 |
+
holographic NLSM, due to the fact that the matter fields backreact to the IR geometry
|
| 881 |
+
and the Kasner exponents are no longer the constant exponents of Schwarzschild black
|
| 882 |
+
hole and instead they depend on T/b, as shown in the first three pictures in Fig. 6.
|
| 883 |
+
Nevertheless, at low enough temperature we see that the Kasner exponents are nearly
|
| 884 |
+
constant.
|
| 885 |
+
0.00
|
| 886 |
+
0.02
|
| 887 |
+
0.04
|
| 888 |
+
0.06
|
| 889 |
+
0.08
|
| 890 |
+
0.10
|
| 891 |
+
-0.298
|
| 892 |
+
-0.296
|
| 893 |
+
-0.294
|
| 894 |
+
-0.292
|
| 895 |
+
-0.290
|
| 896 |
+
-0.288
|
| 897 |
+
-0.286
|
| 898 |
+
T
|
| 899 |
+
b
|
| 900 |
+
pt
|
| 901 |
+
0.00
|
| 902 |
+
0.02
|
| 903 |
+
0.04
|
| 904 |
+
0.06
|
| 905 |
+
0.08
|
| 906 |
+
0.10
|
| 907 |
+
0.182
|
| 908 |
+
0.184
|
| 909 |
+
0.186
|
| 910 |
+
0.188
|
| 911 |
+
0.190
|
| 912 |
+
0.192
|
| 913 |
+
T
|
| 914 |
+
b
|
| 915 |
+
px
|
| 916 |
+
0.00
|
| 917 |
+
0.02
|
| 918 |
+
0.04
|
| 919 |
+
0.06
|
| 920 |
+
0.08
|
| 921 |
+
0.10
|
| 922 |
+
0.916
|
| 923 |
+
0.918
|
| 924 |
+
0.920
|
| 925 |
+
0.922
|
| 926 |
+
T
|
| 927 |
+
b
|
| 928 |
+
pz
|
| 929 |
+
0.00
|
| 930 |
+
0.02
|
| 931 |
+
0.04
|
| 932 |
+
0.06
|
| 933 |
+
0.08
|
| 934 |
+
0.10
|
| 935 |
+
0.902
|
| 936 |
+
0.904
|
| 937 |
+
0.906
|
| 938 |
+
0.908
|
| 939 |
+
0.910
|
| 940 |
+
0.912
|
| 941 |
+
0.914
|
| 942 |
+
T
|
| 943 |
+
b
|
| 944 |
+
τs
|
| 945 |
+
Figure 6: Plots of Kasner exponents and τs for holographic NLSM as a function of T/b when
|
| 946 |
+
M/b = 0.
|
| 947 |
+
14
|
| 948 |
+
|
| 949 |
+
3.2
|
| 950 |
+
Proper time of timelike geodesics
|
| 951 |
+
Similar to the holographic WSM, we can also discuss the proper time from the horizon
|
| 952 |
+
to the singularity in holographic NLSM. In Fig. 7, we show the proper time τs as a
|
| 953 |
+
function of M/b at different temperatures. Again we see that at low temperature, the
|
| 954 |
+
proper time is almost a constant in the topological phase (e.g. within the difference of
|
| 955 |
+
order less than 5‰ between M/b = 0.5 and M/b = 0 at T/b = 0.01), which shows a
|
| 956 |
+
topological behavior under the changes of the systems. Similar to the holographic WSM,
|
| 957 |
+
we could take the operator which encodes the information of τs as the order parameter
|
| 958 |
+
for the topological phase transition in holographic NLSM. In the trivial phase, the proper
|
| 959 |
+
time τs is monotonically decreasing when we increase M/b.
|
| 960 |
+
���
|
| 961 |
+
���
|
| 962 |
+
���
|
| 963 |
+
���
|
| 964 |
+
���
|
| 965 |
+
���
|
| 966 |
+
���
|
| 967 |
+
���
|
| 968 |
+
���
|
| 969 |
+
���
|
| 970 |
+
���
|
| 971 |
+
M
|
| 972 |
+
b
|
| 973 |
+
τs
|
| 974 |
+
Figure 7: Plots of the proper time τs from the horizon to the singularity as a function of M/b
|
| 975 |
+
at different temperatures T/b = 0.05 (red), 0.02 (blue), 0.01 (purple).
|
| 976 |
+
4
|
| 977 |
+
Conclusion and discussion
|
| 978 |
+
We have studied the interior geometries of black holes in two different holographic topo-
|
| 979 |
+
logical semimetals. We find that the singularities of the geometries are of simple Kasner
|
| 980 |
+
form, together with a constant one form gauge potential or constant two form fields.
|
| 981 |
+
In the topological WSM phase, all the Kasner exponents are constant taking values of
|
| 982 |
+
Schwarzschild black hole at low temperature. In the topological NLSM phase, the Kasner
|
| 983 |
+
exponents of the metric fields are also almost constant (the difference is of order less than
|
| 984 |
+
1% at T/b = 0.01), while the Kasner exponent of the scalar field is small and changes
|
| 985 |
+
a bit in the topological phase. Moreover, we find the proper times from the horizon to
|
| 986 |
+
the singularity are nearly constant in both holographic WSM and holographic NLSM.
|
| 987 |
+
These features seem to be of topological in the sense that they stay as constant during
|
| 988 |
+
15
|
| 989 |
+
|
| 990 |
+
the changes of physical parameters of the systems. The proper time in the trivial phases
|
| 991 |
+
of the two holographic semimetal decreases when we increase M/b.
|
| 992 |
+
In addition to the above universal behavior, specific behaviors inside the horizon are
|
| 993 |
+
also found. In the topological phase of holographic WSM, we find the oscillations of
|
| 994 |
+
the matter field φ inside the horizon at low temperature. In other phases we have not
|
| 995 |
+
found any oscillations of fields. The Kasner exponents oscillate in the critical regime
|
| 996 |
+
of holographic WSM. There is no oscillation of background fields in holographic NLSM.
|
| 997 |
+
In the trivial phases of the two holographic semimetals, the Kasner exponents behave
|
| 998 |
+
differently, where the details can be found in Fig. 3 and Fig. 5.
|
| 999 |
+
It would be interesting to connect the topological features of Kasner exponents and
|
| 1000 |
+
the proper times in the topological phases of the two holographic semimetals to the
|
| 1001 |
+
topological invariants. It is known that they can be extracted from the correlators of
|
| 1002 |
+
heavy operators. It is very interesting to determine the precise observables associated
|
| 1003 |
+
to these quantities to understand the role played by topology. This would shed light
|
| 1004 |
+
on the universal theories describing the topological semimetals. Meanwhile, it is also
|
| 1005 |
+
interesting to check the behavior of these physical quantities in the topological phases
|
| 1006 |
+
of other holographic topological semimetals, e.g. [18, 25], to check if they are universal
|
| 1007 |
+
feature of topological semimetals.
|
| 1008 |
+
Acknowledgments
|
| 1009 |
+
We are grateful to Matteo Baggioli, Karl Landsteiner, Ya-Wen Sun, Xin-Meng Wu, Jun-
|
| 1010 |
+
Kun Zhao for useful discussions. This work is supported by the National Natural Science
|
| 1011 |
+
Foundation of China grant No.11875083.
|
| 1012 |
+
A
|
| 1013 |
+
Equations in holographic WSM
|
| 1014 |
+
In this appendix we list the useful equations for calculating the geometries in holographic
|
| 1015 |
+
WSM in section 2.
|
| 1016 |
+
16
|
| 1017 |
+
|
| 1018 |
+
The equations of motion for the action (2.1) are
|
| 1019 |
+
Rab − 1
|
| 1020 |
+
2gab(R + 12) − Tab = 0 ,
|
| 1021 |
+
∇bF ba + αϵabcde(FbcFde + FbcFde) − iq (Φ∗(DaΦ) − Φ(DaΦ)∗) = 0 ,
|
| 1022 |
+
∇bFba + 2αϵabcdeFbcFde = 0 ,
|
| 1023 |
+
DaDaΦ − m2Φ − λΦ∗Φ2 = 0 ,
|
| 1024 |
+
(A.1)
|
| 1025 |
+
where
|
| 1026 |
+
Tab =1
|
| 1027 |
+
2(FacF c
|
| 1028 |
+
b − 1
|
| 1029 |
+
4gabF2) + 1
|
| 1030 |
+
2(FacF c
|
| 1031 |
+
b − 1
|
| 1032 |
+
4gabF 2) + 1
|
| 1033 |
+
2((DaΦ)∗DbΦ + (DbΦ)∗DaΦ)
|
| 1034 |
+
− 1
|
| 1035 |
+
2gab((DcΦ)∗DcΦ + V (Φ))
|
| 1036 |
+
(A.2)
|
| 1037 |
+
and DaΦ = ∂aΦ − iqAaΦ.
|
| 1038 |
+
There are three different scaling symmetries of the system
|
| 1039 |
+
(x, y) → a(x, y) , f → a−2f ;
|
| 1040 |
+
(A.3)
|
| 1041 |
+
z → az , h → a−2h , Az → a−1Az ;
|
| 1042 |
+
(A.4)
|
| 1043 |
+
r → ar , (t, x, y, z) → a−1(t, x, y, z) , (u, f, h) → a2(u, f, h) , Az → aAz .
|
| 1044 |
+
(A.5)
|
| 1045 |
+
For the ansatz (2.2), we have equations
|
| 1046 |
+
u′′ + h′
|
| 1047 |
+
2hu′ −
|
| 1048 |
+
�
|
| 1049 |
+
f ′′ + f ′h′
|
| 1050 |
+
2h
|
| 1051 |
+
�u
|
| 1052 |
+
f = 0 ,
|
| 1053 |
+
f ′′
|
| 1054 |
+
f + u′′
|
| 1055 |
+
2u − f ′2
|
| 1056 |
+
4f 2 + f ′u′
|
| 1057 |
+
fu − 6
|
| 1058 |
+
u + φ2
|
| 1059 |
+
2u
|
| 1060 |
+
�
|
| 1061 |
+
m2 + λ
|
| 1062 |
+
2φ2 − q2A2
|
| 1063 |
+
z
|
| 1064 |
+
h
|
| 1065 |
+
�
|
| 1066 |
+
− A′2
|
| 1067 |
+
z
|
| 1068 |
+
4h + 1
|
| 1069 |
+
2φ′2 = 0 ,
|
| 1070 |
+
1
|
| 1071 |
+
2φ′2 + 6
|
| 1072 |
+
u − u′
|
| 1073 |
+
2u
|
| 1074 |
+
�f ′
|
| 1075 |
+
f + h′
|
| 1076 |
+
2h
|
| 1077 |
+
�
|
| 1078 |
+
− f ′h′
|
| 1079 |
+
2fh − f ′2
|
| 1080 |
+
4f 2 + A′2
|
| 1081 |
+
z
|
| 1082 |
+
4h − φ2
|
| 1083 |
+
2u
|
| 1084 |
+
�
|
| 1085 |
+
m2 + λ
|
| 1086 |
+
2φ2 − q2A2
|
| 1087 |
+
z
|
| 1088 |
+
h
|
| 1089 |
+
�
|
| 1090 |
+
= 0 ,
|
| 1091 |
+
A′′
|
| 1092 |
+
z +
|
| 1093 |
+
�f ′
|
| 1094 |
+
f − h′
|
| 1095 |
+
2h + u′
|
| 1096 |
+
u
|
| 1097 |
+
�
|
| 1098 |
+
A′
|
| 1099 |
+
z − 2q2φ2
|
| 1100 |
+
u
|
| 1101 |
+
Az = 0 ,
|
| 1102 |
+
φ′′ +
|
| 1103 |
+
�f ′
|
| 1104 |
+
f + h′
|
| 1105 |
+
2h + u′
|
| 1106 |
+
u
|
| 1107 |
+
�
|
| 1108 |
+
φ′ − 1
|
| 1109 |
+
u
|
| 1110 |
+
�q2A2
|
| 1111 |
+
z
|
| 1112 |
+
h
|
| 1113 |
+
+ m2 + λφ2�
|
| 1114 |
+
φ = 0 .
|
| 1115 |
+
(A.6)
|
| 1116 |
+
Near the horizon r = rh, the fields can be expanded as follows,
|
| 1117 |
+
u = 4πT(r − rh) + · · · ,
|
| 1118 |
+
f = f1 − f1Az2
|
| 1119 |
+
2m2φ2
|
| 1120 |
+
1 + λφ4
|
| 1121 |
+
1 − 24
|
| 1122 |
+
6Az1q2φ2
|
| 1123 |
+
1
|
| 1124 |
+
(r − rh) + · · · ,
|
| 1125 |
+
h = h1 −
|
| 1126 |
+
�
|
| 1127 |
+
Az1Az2 + h1Az2
|
| 1128 |
+
2m2φ2
|
| 1129 |
+
1 + λφ4
|
| 1130 |
+
1 − 24
|
| 1131 |
+
6Az1q2φ2
|
| 1132 |
+
1
|
| 1133 |
+
�
|
| 1134 |
+
(r − rh) + · · · ,
|
| 1135 |
+
Az = Az1 + Az2(r − rh) + · · · ,
|
| 1136 |
+
φ = φ1 + Az2
|
| 1137 |
+
A2
|
| 1138 |
+
z1q2 + h1(m2 + λφ2
|
| 1139 |
+
1)
|
| 1140 |
+
2Az1h1q2φ2
|
| 1141 |
+
1
|
| 1142 |
+
(r − rh) + · · · ,
|
| 1143 |
+
(A.7)
|
| 1144 |
+
17
|
| 1145 |
+
|
| 1146 |
+
where T =
|
| 1147 |
+
φ2
|
| 1148 |
+
1q2Az1
|
| 1149 |
+
2πAz2 . Note that there is a shift symmetry r → r + α along the radial
|
| 1150 |
+
direction which can be used to fix rh to be any value and we choose rh = 1. There are
|
| 1151 |
+
five free parameters T, f1, h1, Az1, φ1 and we can use the scaling symmetries (A.3, A.4) to
|
| 1152 |
+
fix f1 = 1, h1 = 1 respectively. Then we can shoot three parameters T, Az1, φ1 to obtain
|
| 1153 |
+
the parameters T, M, b of boundary field theory, i.e. the two dimensionless parameters
|
| 1154 |
+
T/b, M/b according the scaling symmetry in (A.5) (we work in unit b = 1).
|
| 1155 |
+
When r → ∞, the UV expansions are
|
| 1156 |
+
u = r2 − M 2
|
| 1157 |
+
3
|
| 1158 |
+
+ M 4(2 + 3λ)
|
| 1159 |
+
18
|
| 1160 |
+
ln r
|
| 1161 |
+
r2 − Mb
|
| 1162 |
+
r2 + · · · ,
|
| 1163 |
+
f = r2 − M 2
|
| 1164 |
+
3
|
| 1165 |
+
+ M 4(2 + 3λ)
|
| 1166 |
+
18
|
| 1167 |
+
ln r
|
| 1168 |
+
r2 + f3
|
| 1169 |
+
r2 + · · · ,
|
| 1170 |
+
h = r2 − M 2
|
| 1171 |
+
3
|
| 1172 |
+
+ M 4(2 + 3λ) + 9b2M 2q2
|
| 1173 |
+
18
|
| 1174 |
+
ln r
|
| 1175 |
+
r2 + h3
|
| 1176 |
+
r2 + · · · ,
|
| 1177 |
+
Az = b − bM 2q2ln r
|
| 1178 |
+
r2 + η
|
| 1179 |
+
r2 + · · · ,
|
| 1180 |
+
φ = M
|
| 1181 |
+
r − (3b2Mq2 + 2M 3 + 3λM 3))
|
| 1182 |
+
6
|
| 1183 |
+
ln r
|
| 1184 |
+
r3 + O
|
| 1185 |
+
r3 + · · · ,
|
| 1186 |
+
(A.8)
|
| 1187 |
+
where h3 =
|
| 1188 |
+
1
|
| 1189 |
+
72M(−72O + 9b2Mq2 + M 3(14 + 9λ)) − 2f3.
|
| 1190 |
+
Note that in order to match the expansion (A.8) we should use the shift symmetry of
|
| 1191 |
+
the system r → r + α which could change the location of the horizon/singularity.
|
| 1192 |
+
B
|
| 1193 |
+
Equations in holographic NLSM
|
| 1194 |
+
In this appendix, we list the calculations for the geometries in holographic NLSM in
|
| 1195 |
+
section 3.
|
| 1196 |
+
The equations of motion for the action (3.1) are
|
| 1197 |
+
Rab − 1
|
| 1198 |
+
2gab(R + 12) − Tab = 0 ,
|
| 1199 |
+
∇bFba + 2αϵabcdeFbcFde = 0 ,
|
| 1200 |
+
∇bF ba + αϵabcde(FbcFde + FbcFde) − iq1 (Φ∗DaΦ − (DaΦ)∗Φ) + q2
|
| 1201 |
+
η ϵabcdeBbcB∗
|
| 1202 |
+
de = 0 ,
|
| 1203 |
+
DaDaΦ − ∂Φ∗V1 − λΦB∗
|
| 1204 |
+
abBab = 0 ,
|
| 1205 |
+
i
|
| 1206 |
+
3ηϵabcdeHcde − m2
|
| 1207 |
+
2Bab − λΦ∗ΦBab = 0 ,
|
| 1208 |
+
(B.1)
|
| 1209 |
+
18
|
| 1210 |
+
|
| 1211 |
+
where
|
| 1212 |
+
Tab = 1
|
| 1213 |
+
2(FacF c
|
| 1214 |
+
b − 1
|
| 1215 |
+
4gabF2) + 1
|
| 1216 |
+
2(FacF c
|
| 1217 |
+
b − 1
|
| 1218 |
+
4gabF 2) + 1
|
| 1219 |
+
2
|
| 1220 |
+
�
|
| 1221 |
+
(DaΦ)∗DbΦ + (DbΦ)∗DaΦ
|
| 1222 |
+
�
|
| 1223 |
+
+ (m2
|
| 1224 |
+
2 + λ|Φ|2)(B∗
|
| 1225 |
+
acB c
|
| 1226 |
+
b + B∗
|
| 1227 |
+
bcB c
|
| 1228 |
+
a ) − 1
|
| 1229 |
+
2gab
|
| 1230 |
+
�
|
| 1231 |
+
(DcΦ)∗DcΦ + V1 + V2 + λ|Φ|2B∗
|
| 1232 |
+
cdBcd�
|
| 1233 |
+
.
|
| 1234 |
+
(B.2)
|
| 1235 |
+
With the ansatz (3.4), the equations are
|
| 1236 |
+
u′′
|
| 1237 |
+
u − f ′′
|
| 1238 |
+
f + h′
|
| 1239 |
+
2h
|
| 1240 |
+
�u′
|
| 1241 |
+
u − f ′
|
| 1242 |
+
f
|
| 1243 |
+
�
|
| 1244 |
+
− 4
|
| 1245 |
+
u(m2
|
| 1246 |
+
2 + λφ2)
|
| 1247 |
+
�B2
|
| 1248 |
+
tz
|
| 1249 |
+
uh + B2
|
| 1250 |
+
xy
|
| 1251 |
+
f 2
|
| 1252 |
+
�
|
| 1253 |
+
= 0 ,
|
| 1254 |
+
u′′
|
| 1255 |
+
2u + f ′′
|
| 1256 |
+
f − f ′2
|
| 1257 |
+
4f 2 + f ′u′
|
| 1258 |
+
fu − 6
|
| 1259 |
+
u + 1
|
| 1260 |
+
u(m2
|
| 1261 |
+
2 + λφ2)
|
| 1262 |
+
�B2
|
| 1263 |
+
tz
|
| 1264 |
+
uh + B2
|
| 1265 |
+
xy
|
| 1266 |
+
f 2
|
| 1267 |
+
�
|
| 1268 |
+
+φ2
|
| 1269 |
+
2u
|
| 1270 |
+
�
|
| 1271 |
+
m2
|
| 1272 |
+
1 + λ1φ2
|
| 1273 |
+
2
|
| 1274 |
+
�
|
| 1275 |
+
+ φ′2
|
| 1276 |
+
2 = 0 ,
|
| 1277 |
+
f ′2
|
| 1278 |
+
4f 2 + f ′h′
|
| 1279 |
+
2fh + u′
|
| 1280 |
+
2u
|
| 1281 |
+
�f ′
|
| 1282 |
+
f + h′
|
| 1283 |
+
2h
|
| 1284 |
+
�
|
| 1285 |
+
− 6
|
| 1286 |
+
u + 1
|
| 1287 |
+
u(m2
|
| 1288 |
+
2 + λφ2)
|
| 1289 |
+
�
|
| 1290 |
+
−B2
|
| 1291 |
+
tz
|
| 1292 |
+
uh + B2
|
| 1293 |
+
xy
|
| 1294 |
+
f 2
|
| 1295 |
+
�
|
| 1296 |
+
+φ2
|
| 1297 |
+
2u
|
| 1298 |
+
�
|
| 1299 |
+
m2
|
| 1300 |
+
1 + λ1φ2
|
| 1301 |
+
2
|
| 1302 |
+
�
|
| 1303 |
+
− 1
|
| 1304 |
+
2φ′2 = 0 ,
|
| 1305 |
+
B′
|
| 1306 |
+
tz − η
|
| 1307 |
+
√
|
| 1308 |
+
h
|
| 1309 |
+
2f (m2
|
| 1310 |
+
2 + λφ2)Bxy = 0 ,
|
| 1311 |
+
B′
|
| 1312 |
+
xy −
|
| 1313 |
+
ηf
|
| 1314 |
+
2
|
| 1315 |
+
√
|
| 1316 |
+
hu
|
| 1317 |
+
(m2
|
| 1318 |
+
2 + λφ2)Btz = 0 ,
|
| 1319 |
+
φ′′ + φ′
|
| 1320 |
+
�u′
|
| 1321 |
+
u + f ′
|
| 1322 |
+
f + h′
|
| 1323 |
+
2h
|
| 1324 |
+
�
|
| 1325 |
+
−
|
| 1326 |
+
�
|
| 1327 |
+
m2
|
| 1328 |
+
1 + λ1φ2 − 2λB2
|
| 1329 |
+
tz
|
| 1330 |
+
uh
|
| 1331 |
+
+ 2λB2
|
| 1332 |
+
xy
|
| 1333 |
+
f 2
|
| 1334 |
+
� φ
|
| 1335 |
+
u = 0 .
|
| 1336 |
+
(B.3)
|
| 1337 |
+
There are three different scaling symmetries of the system
|
| 1338 |
+
(x, y) → a(x, y) , f → a−2f , Bxy → a−2Bxy ;
|
| 1339 |
+
(B.4)
|
| 1340 |
+
z → az , h → a−2h , Btz → a−1Btz ;
|
| 1341 |
+
(B.5)
|
| 1342 |
+
r → ar , (t, x, y, z) → a−1(t, x, y, z) , (u, f, h, Bxy, Btz) → a2(u, f, h, Bxy, Btz) .
|
| 1343 |
+
(B.6)
|
| 1344 |
+
19
|
| 1345 |
+
|
| 1346 |
+
Near the horizon r → rh, the fields can be expanded as follows,
|
| 1347 |
+
u = 4πT(r − rh) + · · · ,
|
| 1348 |
+
f = f1 − 4Bxy2
|
| 1349 |
+
�
|
| 1350 |
+
8B2
|
| 1351 |
+
xy1(m2
|
| 1352 |
+
2 + λφ2
|
| 1353 |
+
1) + f 2
|
| 1354 |
+
1(2m2
|
| 1355 |
+
1φ2
|
| 1356 |
+
1 + λ1φ4
|
| 1357 |
+
1 − 24)
|
| 1358 |
+
�
|
| 1359 |
+
3Bxy1f1η2(m2
|
| 1360 |
+
2 + λφ2
|
| 1361 |
+
1)2
|
| 1362 |
+
(r − rh) + · · · ,
|
| 1363 |
+
h = h1 − 4h1Bxy2
|
| 1364 |
+
�
|
| 1365 |
+
4B2
|
| 1366 |
+
xy1(m2
|
| 1367 |
+
2 + λφ2
|
| 1368 |
+
1) − f 2
|
| 1369 |
+
1(2m2
|
| 1370 |
+
1φ2
|
| 1371 |
+
1 + λ1φ4
|
| 1372 |
+
1 − 24)
|
| 1373 |
+
�
|
| 1374 |
+
3Bxy1f1η2(m2
|
| 1375 |
+
2 + λφ2
|
| 1376 |
+
1)2
|
| 1377 |
+
(r − rh) + · · · ,
|
| 1378 |
+
Bxy = Bxy1 + Bxy2(r − rh) + · · · ,
|
| 1379 |
+
Btz = η√h1Bxy1(m2
|
| 1380 |
+
2 + λφ2
|
| 1381 |
+
1)
|
| 1382 |
+
2f1
|
| 1383 |
+
(r − rh) + · · · ,
|
| 1384 |
+
φ = φ1 + 4Bxy2φ1
|
| 1385 |
+
�
|
| 1386 |
+
2λB2
|
| 1387 |
+
xy1 + f 2
|
| 1388 |
+
1(m2
|
| 1389 |
+
1 + λ1φ2
|
| 1390 |
+
1)
|
| 1391 |
+
�
|
| 1392 |
+
Bxy1f 2
|
| 1393 |
+
1η2(m2
|
| 1394 |
+
2 + λφ2
|
| 1395 |
+
1)2
|
| 1396 |
+
(r − rh) + · · · ,
|
| 1397 |
+
(B.7)
|
| 1398 |
+
where T = Bxy1η2(m2
|
| 1399 |
+
2+λφ2
|
| 1400 |
+
1)2
|
| 1401 |
+
16πBxy2
|
| 1402 |
+
. The strategy of the numerics the same as the holographic
|
| 1403 |
+
WSM. We first use the shift symmetry r → r + α to fix rh = 1. Then we also have five
|
| 1404 |
+
free parameters T, f1, h1, Bxy1, φ1 and we can use the scaling symmetries (B.4, B.5) to
|
| 1405 |
+
fix f1 = 1, h1 = 1 respectively. After that we have only three near horizon parameters
|
| 1406 |
+
T, Bxy1, φ1, from which we obtain T, M, b in the dual field theory, which are equivalently
|
| 1407 |
+
two dimensionless parameters T/b, M/b according the scaling symmetry (B.6).
|
| 1408 |
+
Near the boundary r → ∞, we have
|
| 1409 |
+
u = r2 − 2b2 − M 2
|
| 1410 |
+
3
|
| 1411 |
+
+ 8b4 + M 4(2 + 3λ1)
|
| 1412 |
+
18
|
| 1413 |
+
ln r
|
| 1414 |
+
r2 − Mb
|
| 1415 |
+
r2 + · · · ,
|
| 1416 |
+
f = r2 − M 2
|
| 1417 |
+
3
|
| 1418 |
+
+ 8b4 + M 4(2 + 3λ1)
|
| 1419 |
+
18
|
| 1420 |
+
ln r
|
| 1421 |
+
r2 + f3
|
| 1422 |
+
r2 + · · · ,
|
| 1423 |
+
h = r2 − 2b2 − M 2
|
| 1424 |
+
3
|
| 1425 |
+
+ 8b4 + M 4(2 + 3λ1)
|
| 1426 |
+
18
|
| 1427 |
+
ln r
|
| 1428 |
+
r2 + h3
|
| 1429 |
+
r2 + · · · ,
|
| 1430 |
+
Bxy = br + 2b3 ln r
|
| 1431 |
+
r
|
| 1432 |
+
+ b2
|
| 1433 |
+
r + · · · ,
|
| 1434 |
+
Btz = br − 2b3 ln r
|
| 1435 |
+
r
|
| 1436 |
+
− b (b2 + M 2(1 + λ)) + b2
|
| 1437 |
+
r
|
| 1438 |
+
+ · · · ,
|
| 1439 |
+
φ = M
|
| 1440 |
+
r − M 3(2 + 3λ1)
|
| 1441 |
+
6
|
| 1442 |
+
ln r
|
| 1443 |
+
r3 + O
|
| 1444 |
+
r3 + · · · ,
|
| 1445 |
+
(B.8)
|
| 1446 |
+
where b2 =
|
| 1447 |
+
1
|
| 1448 |
+
48b (−56b4 + 72(2f3 + h3) − 8b2M 2(2 + 3λ) − M 4(14 + 9λ1) + 72MO).
|
| 1449 |
+
Note that to match the expansion (B.8) we should use the shift symmetry r → r + α
|
| 1450 |
+
which could change the location of the horizon/singularity .
|
| 1451 |
+
20
|
| 1452 |
+
|
| 1453 |
+
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|
| 1454 |
+
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7tAzT4oBgHgl3EQfgfwd/content/tmp_files/load_file.txt
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|
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|
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99FST4oBgHgl3EQfbzgH/vector_store/index.pkl
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+
version https://git-lfs.github.com/spec/v1
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|
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|
9NAyT4oBgHgl3EQfqPh6/content/tmp_files/2301.00539v1.pdf.txt
ADDED
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|
| 1 |
+
1
|
| 2 |
+
|
| 3 |
+
|
| 4 |
+
|
| 5 |
+
|
| 6 |
+
|
| 7 |
+
|
| 8 |
+
|
| 9 |
+
|
| 10 |
+
Statistical Machine Translation for Indic
|
| 11 |
+
Languages
|
| 12 |
+
Sudhansu Bala Das, Divyajoti Panda, Tapas Kumar Mishra,
|
| 13 |
+
and Bidyut Kr. Patra
|
| 14 |
+
National Institute of Technology(NIT), Rourkela, Odisha,
|
| 15 |
+
India
|
| 16 |
+
Indian Institute of Technology (IIT), Varanasi, Uttar Pradesh,
|
| 17 |
+
India
|
| 18 |
+
|
| 19 |
+
|
| 20 |
+
Abstract
|
| 21 |
+
Machine Translation (MT) system generally aims at automatic
|
| 22 |
+
representation of source language into target language retaining the
|
| 23 |
+
originality of context using various Natural Language Processing (NLP)
|
| 24 |
+
techniques. Among various NLP methods, Statistical Machine Trans-
|
| 25 |
+
lation (SMT) is a very popular and successful architecture used for
|
| 26 |
+
both low as well as high-resource languages. SMT uses probabilis-
|
| 27 |
+
tic and statistical techniques to analyze information and conversion.
|
| 28 |
+
This paper canvasses about the development of bilingual SMT mod-
|
| 29 |
+
els for translating English to fifteen low-resource Indian Languages
|
| 30 |
+
(ILs) and vice versa. At the outset, all 15 languages are briefed with
|
| 31 |
+
a short description related to our experimental need. Further, a de-
|
| 32 |
+
tailed analysis of Samanantar and OPUS dataset for model building,
|
| 33 |
+
along with standard benchmark dataset (Flores-200) for fine-tuning
|
| 34 |
+
and testing, is done as a part of our experiment. Different preprocess-
|
| 35 |
+
ing approaches are proposed in this paper to handle the noise of the
|
| 36 |
+
dataset. To create the system, MOSES open-source SMT toolkit is
|
| 37 |
+
explored. “Distance” reordering is utilized with the aim to understand
|
| 38 |
+
the rules of grammar and context-dependent adjustments through a
|
| 39 |
+
|
| 40 |
+
2
|
| 41 |
+
|
| 42 |
+
|
| 43 |
+
|
| 44 |
+
|
| 45 |
+
|
| 46 |
+
phrase reordering categorization framework. In our experiment, the
|
| 47 |
+
quality of the translation is evaluated using standard metrics such as
|
| 48 |
+
BLEU, METEOR, and RIBES.
|
| 49 |
+
|
| 50 |
+
1 Introduction
|
| 51 |
+
Technology reaches new heights through its journey from the origins of ideas
|
| 52 |
+
to their full-scale practical implementation. One such journey is heading to-
|
| 53 |
+
wards elimination of language barrier in order to establish a seamless social
|
| 54 |
+
communication in every domain. In this regard, advancement on relevant
|
| 55 |
+
fields such as Natural Language Processing (NLP), Machine Learning (ML)
|
| 56 |
+
and Artificial Intelligence (AI) based Language Modelling (LM) significantly
|
| 57 |
+
contributes for evolving a flawless automatic Machine Translation (MT) sys-
|
| 58 |
+
tem (Dorr et al ( 2004)). Irrespective of various heuristic approaches to
|
| 59 |
+
maintain both lexical and contextual interpretation of source language(s)
|
| 60 |
+
onto the translated target language(s), it is still challenging to cope with
|
| 61 |
+
required fluency, adequacy, accent, and overall accuracy (Chapelle et al (
|
| 62 |
+
2010)). However, it is feasible with the advent of modern NLP (AI-based)
|
| 63 |
+
approaches wherein a high-quality and high resource (i.e. large quantity
|
| 64 |
+
of corpora available) parallel corpus (translation pairs in source and target
|
| 65 |
+
languages) is required to train a good translation system. Hence, for high-
|
| 66 |
+
resource languages having massive digital footprint across the globe, MT sys-
|
| 67 |
+
tems prove to be quite efficient with adequate training. On the other hand,
|
| 68 |
+
it becomes very complicated for low-resource languages suffering from uni-
|
| 69 |
+
versal recognition and scanty digital presence. Such imbalance often leads to
|
| 70 |
+
poor-quality translation in presence of low-resource language(s) in the form
|
| 71 |
+
of either target or source. Therefore, MT systems need to understand the
|
| 72 |
+
syntax (rules to combine words), semantics (meaning of words and combi-
|
| 73 |
+
nations), and morphology (rules to cover morphemes - smallest meaningful
|
| 74 |
+
units - into words) of such low-resource languages (Somers (2011)).
|
| 75 |
+
Based on the heuristic paradigms, MT models are classified into rule-based
|
| 76 |
+
(RBMT), example-based (EBMT), statistical (SMT), and neural (NMT) sys-
|
| 77 |
+
tems (Tripathi et al (2010)). Each has its own advantages and disadvantages.
|
| 78 |
+
RBMT models follow a set of rules to define a language and the interaction
|
| 79 |
+
between different linguistic devices (words, phrases, sentences) in the lan-
|
| 80 |
+
guage (Jussà et al (2012), Michael et al (2000)). These sets of rules and
|
| 81 |
+
systems defined for a translation in a language pair are hard-coded on the
|
| 82 |
+
|
| 83 |
+
3
|
| 84 |
+
|
| 85 |
+
|
| 86 |
+
|
| 87 |
+
|
| 88 |
+
|
| 89 |
+
machine. The linguistic information used in an RBMT model is mainly
|
| 90 |
+
the target and source languages collected from unilingual (one language),
|
| 91 |
+
bilingual (two languages), or multilingual (more than two languages) dic-
|
| 92 |
+
tionaries. In addition, the model also uses grammar covering the syntactic,
|
| 93 |
+
semantic, and morphological regularities of each language. However, a well-
|
| 94 |
+
built RBMT model requires highly skilled and expert human labour due to
|
| 95 |
+
its complexity making it hard to build. In addition, the ambiguous proper-
|
| 96 |
+
ties of languages make them prone to take more time and efforts to resolve,
|
| 97 |
+
especially in large and complex models. RBMT models require a lot of effort
|
| 98 |
+
to be made functional in day-to-day life. Hence, the need for more efficient
|
| 99 |
+
translation systems than RBMT still persists. EBMT methods make use of a
|
| 100 |
+
large number of translation examples (John (2005)). Notably, EBMT mod-
|
| 101 |
+
els make use of bilingual corpora manipulation, i.e. the breaking down of
|
| 102 |
+
a bilingual corpus into smaller parts, translating those parts into the target
|
| 103 |
+
language, and recompiling it to form whole translated sentences. They do
|
| 104 |
+
not account much for the syntax, semantic and morphological analysis of the
|
| 105 |
+
target and source language (like RBMT models). In contrast, SMT is better
|
| 106 |
+
when compared to RBMT and EBMT models, as it does not require human
|
| 107 |
+
intervention (Adam (2008)). It is a way of translation wherein a statistical-
|
| 108 |
+
based learning algorithm is applied to a large bilingual corpus that helps
|
| 109 |
+
the machine learn the translation. This method also enables the machine to
|
| 110 |
+
translate sentences not encountered by the machine during its training and
|
| 111 |
+
testing. The objective of SMT is to convert an input word sequence from the
|
| 112 |
+
source language into the target language. It has dominated academic MT
|
| 113 |
+
research and a portion of the commercial MT sector in less than two decades.
|
| 114 |
+
On the other hand, neural machine translation (NMT) is performed using a
|
| 115 |
+
neural network (NN) (Stasimioti (2020)). Unlike SMT, NMT does not have a
|
| 116 |
+
distinct translation model, language model, or model for reordering. Instead,
|
| 117 |
+
it has a single sequence model that determines one word at a time. The pre-
|
| 118 |
+
diction is based on the source sentence effort previously generated sequence
|
| 119 |
+
in the target language. NMT is a deep learning-based method of machine
|
| 120 |
+
learning that utilizes a large NN that relies on word vector representations.
|
| 121 |
+
Even though the NMT has achieved remarkable results in a few trans-
|
| 122 |
+
lation experiments using high-resource language, researchers are unsure if
|
| 123 |
+
the NMT could actually replace SMT and if its success would extend to
|
| 124 |
+
other tasks. Eventually, the experiment of (Michał (2016)) on the corpus
|
| 125 |
+
of the United Nations (consisting of 15 low-resource languages) brings the
|
| 126 |
+
fact. From the result of his experiment, it is evident that the performance of
|
| 127 |
+
|
| 128 |
+
4
|
| 129 |
+
|
| 130 |
+
|
| 131 |
+
|
| 132 |
+
|
| 133 |
+
|
| 134 |
+
SMT is better than that of NMT for the majority of cases, as measured by
|
| 135 |
+
BLEU score. Many researchers (Lohar et al (2019), Zhou et al (2017), Wang
|
| 136 |
+
et al (2017), Castilho et al (2017)) have pointed out various disadvantages
|
| 137 |
+
of NMT over SMT using low resource language, such as the fact that NMT
|
| 138 |
+
requires more corpus and resources than SMT. In comparison with SMT,
|
| 139 |
+
NMT training typically takes longer. Additionally, research has shown that
|
| 140 |
+
when there is a domain incompatibility between testing and training data,
|
| 141 |
+
SMT performance is superior to that of NMT (Xing et al (2018), Mahata et
|
| 142 |
+
al (2018)). Long sentences are another area where SMT excels.
|
| 143 |
+
English and ILs are languages with less parallel text data, which motivates us
|
| 144 |
+
to work with ILs. This research examines the effectiveness of SMT systems on
|
| 145 |
+
low-resource language pairs, of which many are rarely worked on. The dataset
|
| 146 |
+
used in our experiment for all fifteen Indian languages is tested for the first
|
| 147 |
+
time for all languages using SMT. Hence, the objective of this work is to build
|
| 148 |
+
an MT system using SMT for languages such as Assamese (AS), Malayalam
|
| 149 |
+
(ML), Bengali (BN), Marathi (MR), Gujarati (GU), Kannada (KN), Hindi
|
| 150 |
+
(HI), Oriya (OR), Punjabi (PA), Telugu (TE), Sindhi (SD), Sinhala (SI),
|
| 151 |
+
Nepali (NE), Tamil (TA), and Urdu (UR) to English (EN) and vice versa and
|
| 152 |
+
to check the effectiveness of SMT with low-resource language pairs.
|
| 153 |
+
Our main goal is to develop an MT system for low-resource languages, i.e., ILs,
|
| 154 |
+
that can serve as a baseline system. The following is a summary of our
|
| 155 |
+
work’s main contributions:
|
| 156 |
+
• To the best of our knowledge, this work is the first attempt to use SMT
|
| 157 |
+
with the Samanantar and OPUS Dataset to investigate the MT for all
|
| 158 |
+
fifteen IL-EN and EN-IL pairs (both directions), including both the
|
| 159 |
+
Dravidian and Indo-Aryan groups.
|
| 160 |
+
• To bring forth the linguistic approach of ILs in terms of translation.
|
| 161 |
+
Scripts, writing style, and grammar with proper examples are also dis-
|
| 162 |
+
cussed.
|
| 163 |
+
• Various data filtration methods are investigated in order to clean the
|
| 164 |
+
data and improve translation quality.
|
| 165 |
+
• Distance-based reordering is utilized to check the translation quality of
|
| 166 |
+
ILs.
|
| 167 |
+
|
| 168 |
+
5
|
| 169 |
+
|
| 170 |
+
|
|
| 171 |
+
|
|
| 172 |
+
|
| 173 |
+
|
| 174 |
+
|
| 175 |
+
|
| 176 |
+
• Better realistic assessment of translation quality is possible from the
|
| 177 |
+
presentation of results, as obtained using different automated metrics
|
| 178 |
+
like BLEU, METEOR, and RIBES.
|
| 179 |
+
This paper is arranged as follows. Subsections 1.1 and 1.2 give some
|
| 180 |
+
insight into SMT and cover the ILs used for our experiments. In Section 2,
|
| 181 |
+
some prominent works on SMT and NMT using ILs are described. The
|
| 182 |
+
experimental framework, including an overview of the dataset and method-
|
| 183 |
+
ology, is explained in Section 3. Section 4 narrates some of the prominent
|
| 184 |
+
metrics used for MT evaluation. Results are presented in Section 5 followed by
|
| 185 |
+
the conclusion and future direction in Section 6.
|
| 186 |
+
|
| 187 |
+
1.1 SMT
|
| 188 |
+
Statistical Machine Tramslation (SMT) is dependent on statistical methods
|
| 189 |
+
(Philipp et al (2007), Richard et al (2002), Mary et al (2011) ). It is a data-
|
| 190 |
+
driven technique that makes use of parallel-aligned corpora. It utilizes
|
| 191 |
+
mathematical equations to calculate the likelihood of source-to-target lan-
|
| 192 |
+
guage translation. Probability P (Tl Si) is assigned by SMT. Here Tl is the target
|
| 193 |
+
language and Si is the source input. It utilizes Bayes’ theorem to
|
| 194 |
+
determine the maximum probability P (Tl|Si), which is as follows:
|
| 195 |
+
P (Tl | Si) ∝ P (Tl)P (Si | Tl)
|
| 196 |
+
(1)
|
| 197 |
+
SMT consists of three phases: the language model(LM) P (Tl) for target
|
| 198 |
+
language probability calculation, the translation model(TM) P (Si Tl) for
|
| 199 |
+
conditional probability estimation of the target to the source language, and the
|
| 200 |
+
decoder model (DM), which searches among possible source sentences the
|
| 201 |
+
one which maximizes probabilities (Kumawat et al (2014)).
|
| 202 |
+
To calculate the probability of a sentence, the LM utilizes the n-gram model. It
|
| 203 |
+
assigns the probability of a single word to the last n words that come before it
|
| 204 |
+
in the sentence and estimates the translation’s likelihood. The chain rule aids
|
| 205 |
+
in breaking down the sentence into conditional probability products.
|
| 206 |
+
|
| 207 |
+
P (s) = P (w1, w2, w3, ..., wn)
|
| 208 |
+
= P (w1)P (w2|w1)P (w3|w1w2)P (w4|w1w2w3)...P (wn|w1w2...wn−1)
|
| 209 |
+
= P (w1)P (w2|w1)P (w3|w1w2)P (w4|w1w2w3)...P (wn|w1w2...wn−k)
|
| 210 |
+
(2)
|
| 211 |
+
Where, P (s) is the probability of the sentence s, consisting of words w1, w2,
|
| 212 |
+
..., wn, assuming a k-gram model. It utilizes the bilingual parallel corpus
|
| 213 |
+
|
| 214 |
+
6
|
| 215 |
+
|
| 216 |
+
|
| 217 |
+
|
| 218 |
+
|
| 219 |
+
|
| 220 |
+
of the desired language pair. This is accomplished by calculating the like-
|
| 221 |
+
lihood of words or phrases extracted from sentences. The DM is the final
|
| 222 |
+
and most crucial phase of SMT. It assists in the selection of words with the
|
| 223 |
+
highest probability to be translated by maximizing the likelihood, i.e.
|
| 224 |
+
P (Tl)P (Si | Tl).
|
| 225 |
+
1.2 Language preference
|
| 226 |
+
India is a multilingual nation where people from various states use a variety of
|
| 227 |
+
regional tongues. Such diversity of language brings difficulty in commu-
|
| 228 |
+
nicating with one another for information exchange. Further, limitations in
|
| 229 |
+
public communication also bring inconvenience to share feelings, thoughts,
|
| 230 |
+
opinions and facts, as well as to deal with business purposes. Moreover, there
|
| 231 |
+
are many helpful resources available on the internet in English but many In-
|
| 232 |
+
dians struggle to take benefit of those due to language barriers. Hence, it is
|
| 233 |
+
crucial to have an easy translation solution for regional languages to support
|
| 234 |
+
effective communication and to help utilising global resources. To make it
|
| 235 |
+
possible, technological innovation are continuing to find out efficient methods
|
| 236 |
+
for a flawless translation using machines, because it is impractical to have hu-
|
| 237 |
+
man translators everywhere. For machine translation, an enormous amount
|
| 238 |
+
of resources is required for training with a proper knowledge-base (rules) for
|
| 239 |
+
better efficiency so as to fulfill the demand of a flawless translation solu-
|
| 240 |
+
tion. For translation, understanding the meaning of words is important, but
|
| 241 |
+
words are not enough to constitute a language as a whole. They must be
|
| 242 |
+
used in sentence construction that adheres to strict grammar rules and every
|
| 243 |
+
language is having its own writing style. In our work, 15 commonly spoken
|
| 244 |
+
languages (over various regions of India) are chosen. Table 1 describes the
|
| 245 |
+
languages used in our experiments with their linguistic features (ethnologue
|
| 246 |
+
(2022)). A short introduction about them in terms of translation is given
|
| 247 |
+
below.
|
| 248 |
+
English(EN)
|
| 249 |
+
English language is the primary language of roughly 45 countries and
|
| 250 |
+
is spoken by nearly 1,132 million people. It is written in Roman script,
|
| 251 |
+
which uses both uppercase and lowercase characters. English uses the
|
| 252 |
+
subject-verb-object structure. For example (expl1), “The poor man
|
| 253 |
+
took food”, and (expl2) “food took the poor man”. When the position
|
| 254 |
+
|
| 255 |
+
7
|
| 256 |
+
|
| 257 |
+
|
| 258 |
+
|
| 259 |
+
|
| 260 |
+
|
| 261 |
+
of the subject changes in the preceding sentences, the significance and
|
| 262 |
+
meaning of the English sentence change.
|
| 263 |
+
Assamese(AS)
|
| 264 |
+
Over 15 million native Assamese speakers live in the state of Assam in
|
| 265 |
+
the northeastern region of India. It is one of Assam’s official languages.
|
| 266 |
+
Additionally, it is spoken in various regions of other northeastern In-
|
| 267 |
+
dian states. It uses the Bengali-Assamese script and is written left to
|
| 268 |
+
right. It also follows the SOV format. “Gita is eating mango” is an
|
| 269 |
+
English sentence that when translated into Assamese became গীতাই আম
|
| 270 |
+
খাই আআছ which follows subject object verb format. গীতাই (Gita,
|
| 271 |
+
subject), আম(mango, object) and খাই আআছ(is eating, verb).
|
| 272 |
+
Malayalam(ML)
|
| 273 |
+
People in Kerala and a few societies in Karnataka and Tamil Nadu use
|
| 274 |
+
Malayalam for communication. This language is spoken by about 35
|
| 275 |
+
million citizens. It uses the SOV style of writing and a nominative-
|
| 276 |
+
accusative case marking sequence. It is written in Malayalam script in
|
| 277 |
+
left-to-right fashion. Sentence like സീതയ്ക്ക് ചിത്തരചന ഇഷ്ട മാണ്
|
| 278 |
+
which in English became “Sita loves drawing”. Here the word
|
| 279 |
+
സീതയ്ക്ക്
|
| 280 |
+
(Sita,Subject), ഇഷ്ടമാണ്
|
| 281 |
+
(loves,Verb) and ചിത്തര
|
| 282 |
+
ചന(drawing,Object).
|
| 283 |
+
Bengali(BN)
|
| 284 |
+
It is the primary language of Bangladesh and the second most spoken
|
| 285 |
+
language in India. Over 265 million people use it as their primary
|
| 286 |
+
or second language. Approximately 11 million Bengali speakers exist
|
| 287 |
+
in Bangladesh. In India, states such as Assam, Tripura, and West
|
| 288 |
+
Bengal use this language. It is a member of the Indo-Aryan family. In
|
| 289 |
+
Bengali sentences, the standard word order is Subject-Object-Verb. For
|
| 290 |
+
example, in sentence আ রাি জ ভাত খায় which in English is “Rosy eats
|
| 291 |
+
rice ”. Here আ রাি জ (Rosy, Subject), ভাত (Rice, object) and খায়
|
| 292 |
+
(Eats,Verb).
|
| 293 |
+
Marathi(MR)
|
| 294 |
+
Marathi is associated with the Sanskrit-derived group of Indian lan-
|
| 295 |
+
guages and is used by 95 million people in India for communication,
|
| 296 |
+
primarily in the central and western regions. The fourth most widely
|
| 297 |
+
spoken language in India is Marathi, which has a sizable native-speaker
|
| 298 |
+
|
| 299 |
+
8
|
| 300 |
+
|
| 301 |
+
|
| 302 |
+
|
| 303 |
+
|
| 304 |
+
|
| 305 |
+
population. Similar to Hindi and Nepali, Marathi is written in the De-
|
| 306 |
+
vanagari script in left-to-right order. It follows the Subject-Object-Verb
|
| 307 |
+
order. For example, the sentence तो दध ि पतो, which means “He drinks
|
| 308 |
+
milk.” in English, has तो दध
|
| 309 |
+
ject), and ि पतो(drinks,
|
| 310 |
+
verb).
|
| 311 |
+
Gujarati(GU)
|
| 312 |
+
ि पतो where तो(He, subject),
|
| 313 |
+
दध
|
| 314 |
+
(Milk, ob-
|
| 315 |
+
Gujarati is spoken by 45 million citizens in Gujarat and is associated
|
| 316 |
+
with the Indo-Aryan group. It uses the SOV writing style and is drafted
|
| 317 |
+
from left to right in Gujarati script. For example, in the sentence તે
|
| 318 |
+
આઈસ્ક્રીમ ખાય છે. which in English is “He is eating ice cream.” where તે
|
| 319 |
+
is subject, આઈસ્ક્રીમ is an object and verb is ખાય છે.
|
| 320 |
+
Kannada (KN)
|
| 321 |
+
Karnataka’s official language is Kannada, which is also widely used
|
| 322 |
+
in other parts of India. In India, about 36 million people speak and
|
| 323 |
+
write Kannada. Despite being a Dravidian language with extensive
|
| 324 |
+
historical literature, Kannada has few computational linguistics re-
|
| 325 |
+
sources, making it challenging to study the language’s literature due
|
| 326 |
+
to its semantic and syntactic diversity. Subject-Object-Verb is the way
|
| 327 |
+
the Kannada language is structured. Kannada is a highly agglutina-
|
| 328 |
+
tive language. It uses the left-to-right Kannada script For example,
|
| 329 |
+
ರಾಮ ಶಾಲೆಗೆ ಹೋದ(SOV) is in English is “Rama went to school”. Here,
|
| 330 |
+
ರಾಮ(Rama, Subject), ಶಾಲೆ(school, object), and ಹೋದರು(went, verb).
|
| 331 |
+
Hindi(HI)
|
| 332 |
+
Hindi is one of the official and national languages of India. There are
|
| 333 |
+
more than 615 million people who use Hindi as their primary language,
|
| 334 |
+
and even more than 341 million who speak it as a second language.
|
| 335 |
+
However, the sentence structure is Subject Object Verb as shown in
|
| 336 |
+
the example: गीता स्क ल जाती है। is in English is “Geeta goes to school”. In
|
| 337 |
+
this sentence, गीता (Gita ,Subject), स्क ल (School, Object) and जाती
|
| 338 |
+
है(Goes, Verb). The Indian Constitution mandates that Hindi written
|
| 339 |
+
in Devanagari be used as the Union’s official language.
|
| 340 |
+
Oriya(OR)
|
| 341 |
+
The Oriya language is the primary language of Odisha, a state in east-
|
| 342 |
+
ern India. Oriya belongs to the Eastern Indo-Aryan group of languages.
|
| 343 |
+
|
| 344 |
+
9
|
| 345 |
+
|
| 346 |
+
Its standard format is subject-object-verb (SOV) and is written in the
|
| 347 |
+
|
| 348 |
+
Odia script from left to right.
|
| 349 |
+
Punjabi (PA)
|
| 350 |
+
Punjabi text is written in a subject-object-verb format and is spoken
|
| 351 |
+
in India and Pakistan, and a few small groups in the United Kingdom,
|
| 352 |
+
United Arab Emirates, Malaysia, the United States, South Africa, and
|
| 353 |
+
Canada. It is written in two scripts: the western Perso-Arabic Shah-
|
| 354 |
+
mukhi script and the eastern Gurmukhi script. Gurmukhi is drafted
|
| 355 |
+
from left to right, whereas Shahmukhi is written in the opposite direc-
|
| 356 |
+
tion. ਅਸ ੀਂ ਭਾਰਤ ਹਾੀਂ is in English “We are Indians” where ਅਸ ੀਂ(We,Sub-
|
| 357 |
+
ject), ਭਾਰਤ (Are,Verb) and ਹਾੀਂ (Indians,Object).
|
| 358 |
+
Telugu(TE)
|
| 359 |
+
Telugu is the official language of two Indian states in the south: Andhra
|
| 360 |
+
Pradesh and Telangana. It is also spoken by the Telugu-speaking im-
|
| 361 |
+
migrant communities in the United States, Canada, and the United
|
| 362 |
+
Kingdom. Text structure in Telugu takes the form of a subject-object-
|
| 363 |
+
verb and from left to right.ఆమె నన్ను కొటి్టంది in English “she beat
|
| 364 |
+
me” where ఆమె(she, Subject), నన్ను (Me, Object) and కొటి్టంది(beat,
|
| 365 |
+
Verb).
|
| 366 |
+
Sindhi(SD)
|
| 367 |
+
Sindhi is a language spoken by 25 million speakers in Pakistan and 5
|
| 368 |
+
million in India. It is written in a modified Perso-Arabic script in Pak-
|
| 369 |
+
istan (right-to-left), whereas it is written in a variety of scripts in India,
|
| 370 |
+
like Devanagari, Khudabadi, and Gurmukhi (left-to-right). It follows the
|
| 371 |
+
Subject-Object-Verb format. For example, the sentence “Partha
|
| 372 |
+
loves books” is رٿﭘﺎ ﮐﻲ ﺘﺎﺑﻦڪ ﻦﺳﺎ رﭘﻴﺎ ﻫﻲآ where ٿﺎرﭘﺎ(Partha, subject),
|
| 373 |
+
ﮐﻲ ﺘﺎﺑﻦڪ (books, object) and ﻦﺳﺎ رﭘﻴﺎ ﻫﻲآ (loves, verb).
|
| 374 |
+
Nepali(NE)
|
| 375 |
+
It is official language and the lingua franca in Nepal, and also spoken
|
| 376 |
+
by some communities in India. Nepali is written in left-to-right De-
|
| 377 |
+
vanagari script. It is a language written in Subject-Object-Verb order For
|
| 378 |
+
example, “Sita ate apples” when converted to the Nepali language
|
| 379 |
+
|
| 380 |
+
10
|
| 381 |
+
|
| 382 |
+
|
| 383 |
+
|
| 384 |
+
|
| 385 |
+
|
| 386 |
+
becomes सीताले स्याउ खाइन्. Here, सीताले(Sita, subject), स्याउ(apples,
|
| 387 |
+
object) and खाइन्(ate, verb).
|
| 388 |
+
Sinhala(SI)
|
| 389 |
+
The majority of Sri Lankans speak Sinhala as their first language. Sin-
|
| 390 |
+
hala is an Indo-Aryan language that differs from English in terms of
|
| 391 |
+
grammatical structure, morphological variation, and subject-object-
|
| 392 |
+
verb (SOV) word order. It is written in right-to-left Sinhala script.
|
| 393 |
+
A sentence like “Pavan writes a letter” is in Sinhala is පවන් ලිපියක්
|
| 394 |
+
ලියයි where පවන්(Pavan, subject), ලිපියක්(a letter, object) and
|
| 395 |
+
ලියයි(writes, verb).
|
| 396 |
+
Tamil(TA)
|
| 397 |
+
Tamil is a language spoken primarily in Tamil Nadu, a state in southern
|
| 398 |
+
India, as well as in countries with a large Tamil diaspora, which includes
|
| 399 |
+
Sri Lanka, Malaysia, and Singapore, to name a few. The phonological
|
| 400 |
+
differences exist within Tamil Nadu between southern, western, and
|
| 401 |
+
northern speech. Tamil is a Dravidian language of the southern branch,
|
| 402 |
+
with a rich literary tradition dating back over 2000 years. Tamil spoken
|
| 403 |
+
in India and Sri Lanka are two different dialects. It uses the Subject
|
| 404 |
+
Object Verb format. For example sentence: “I like paintings” in Tamil
|
| 405 |
+
becomes எனக்கு ஓவியங்கள் பிடிக்கும் where the Iஎனக்கு (I,
|
| 406 |
+
Subject), விலங்குகள் (Paintings, Object) and பிடிக்கும் (Like,
|
| 407 |
+
Verb).
|
| 408 |
+
Urdu(UR)
|
| 409 |
+
It is Pakistan’s national language and is also spoken widely in India.
|
| 410 |
+
In Pakistan and India, Urdu is spoken by over 170 million citizens and is
|
| 411 |
+
also spoken in some communities in the United Kingdom, the United
|
| 412 |
+
States, and the United Arab Emirates. Script for Urdu is a modified
|
| 413 |
+
and revised version of the Perso-Arabic script. Urdu writing structure is
|
| 414 |
+
Subject Object Verb. For example “she reads a book” which in Urdu is
|
| 415 |
+
وہ ﯾﮏا بﮐﺘﺎ ﭘﮍﻫﺘﯽ ۔ہﮯ where وہ(she, Subject), ﯾﮏا بﮐﺘﺎ(book, object) and
|
| 416 |
+
ﭘﮍﻫﺘﺎ ہﮯ(reads, verb).
|
| 417 |
+
|
| 418 |
+
11
|
| 419 |
+
|
| 420 |
+
|
| 421 |
+
|
| 422 |
+
|
| 423 |
+
|
| 424 |
+
Table 1: Linguistic Features of Languages Used in MT Experiments
|
| 425 |
+
|
| 426 |
+
|
| 427 |
+
Languages
|
| 428 |
+
Script
|
| 429 |
+
Word
|
| 430 |
+
Order
|
| 431 |
+
Family
|
| 432 |
+
Number
|
| 433 |
+
of Speakers
|
| 434 |
+
(in millions)
|
| 435 |
+
Writing
|
| 436 |
+
Direction
|
| 437 |
+
Assamese (AS)
|
| 438 |
+
Bengali
|
| 439 |
+
SOV
|
| 440 |
+
Indo-European
|
| 441 |
+
15
|
| 442 |
+
left to right
|
| 443 |
+
Malayalam (ML)
|
| 444 |
+
Malayalam
|
| 445 |
+
SOV
|
| 446 |
+
Dravidian
|
| 447 |
+
38
|
| 448 |
+
left to right
|
| 449 |
+
Bengali (BN)
|
| 450 |
+
Bengali
|
| 451 |
+
SOV
|
| 452 |
+
Indo-European
|
| 453 |
+
265
|
| 454 |
+
left to right
|
| 455 |
+
Marathi (MR)
|
| 456 |
+
Devanagari
|
| 457 |
+
SOV
|
| 458 |
+
Indo-European
|
| 459 |
+
95
|
| 460 |
+
left to right
|
| 461 |
+
Gujarati (GU)
|
| 462 |
+
Gujarati
|
| 463 |
+
SOV
|
| 464 |
+
Indo-European
|
| 465 |
+
60
|
| 466 |
+
left to right
|
| 467 |
+
Kannada (KN)
|
| 468 |
+
Kannada
|
| 469 |
+
SOV
|
| 470 |
+
Dravidian
|
| 471 |
+
36
|
| 472 |
+
left to right
|
| 473 |
+
Hindi (HI)
|
| 474 |
+
Devanagari
|
| 475 |
+
SOV
|
| 476 |
+
Indo-European
|
| 477 |
+
615
|
| 478 |
+
left to right
|
| 479 |
+
Oriya (OR)
|
| 480 |
+
Oriya
|
| 481 |
+
SOV
|
| 482 |
+
Indo-European
|
| 483 |
+
38
|
| 484 |
+
left to right
|
| 485 |
+
Punjabi (PA)
|
| 486 |
+
Perso-Arabic,
|
| 487 |
+
Gurmukhi
|
| 488 |
+
SOV
|
| 489 |
+
Indo-European
|
| 490 |
+
125
|
| 491 |
+
right to left
|
| 492 |
+
left to right
|
| 493 |
+
Telugu (TE)
|
| 494 |
+
Telugu
|
| 495 |
+
SOV
|
| 496 |
+
Dravidian
|
| 497 |
+
93
|
| 498 |
+
left-to-right
|
| 499 |
+
Sindhi (SD)
|
| 500 |
+
Devanagari
|
| 501 |
+
Perso -Arabic
|
| 502 |
+
SOV
|
| 503 |
+
Indo-European
|
| 504 |
+
25
|
| 505 |
+
left to right
|
| 506 |
+
right to left
|
| 507 |
+
Sinhala (SI)
|
| 508 |
+
Sinhala
|
| 509 |
+
SOV
|
| 510 |
+
Indo-European
|
| 511 |
+
17
|
| 512 |
+
left to right
|
| 513 |
+
Nepali (NE)
|
| 514 |
+
Devanagari
|
| 515 |
+
SOV
|
| 516 |
+
Indo-European
|
| 517 |
+
24
|
| 518 |
+
left to right
|
| 519 |
+
Tamil(TA)
|
| 520 |
+
Tamil
|
| 521 |
+
SOV
|
| 522 |
+
Dravidian
|
| 523 |
+
81
|
| 524 |
+
left to right
|
| 525 |
+
Urdu (UR)
|
| 526 |
+
Urdu
|
| 527 |
+
SOV
|
| 528 |
+
Indo-European
|
| 529 |
+
170
|
| 530 |
+
right to left
|
| 531 |
+
English (EN)
|
| 532 |
+
Roman
|
| 533 |
+
SVO
|
| 534 |
+
Indo-European
|
| 535 |
+
1,132
|
| 536 |
+
left to right
|
| 537 |
+
|
| 538 |
+
2 Related Work
|
| 539 |
+
A few works on SMT using some Indic Languages are discussed in this sec-
|
| 540 |
+
tion.
|
| 541 |
+
(Dasgupta et al (2004)) has discussed a technique for English (EN) to Bengali
|
| 542 |
+
(BN) MT that utilizes the syntax of EN sentences to BN while minimizing
|
| 543 |
+
the time of translation. In the process to create the target sentences, a dic-
|
| 544 |
+
tionary is used to know the object and subject, as well as other entities like
|
| 545 |
+
person and number in their work.
|
| 546 |
+
English-to-Hindi (EN-HI) SMT system has been created by (Ananthakrish-
|
| 547 |
+
nan et al (2009)) using morphological and syntactic pre-processing in SMT
|
| 548 |
+
|
| 549 |
+
12
|
| 550 |
+
|
| 551 |
+
|
| 552 |
+
|
| 553 |
+
|
| 554 |
+
|
| 555 |
+
model. In their work, the suffixes in HI language are segmented for mor-
|
| 556 |
+
phological processing before rearranging the EN source sentences as per HI
|
| 557 |
+
syntax.
|
| 558 |
+
In 2010, research has been conducted by (Zbib et al (2010)) at MIT, USA,
|
| 559 |
+
using the grammatical structures in statistical machine translation with the
|
| 560 |
+
Newswire corpus for Arabic to EN language to give better translation results.
|
| 561 |
+
Work on Kannada-to-English MTS with SMT, by (Kumar et al (2015)), using
|
| 562 |
+
Bible corpus on 20,000 sentences shows a remarkable feat with 14.5 BLEU
|
| 563 |
+
score which is even supported by (Papineni et al (2002)).(Kaur et al (2011))
|
| 564 |
+
has presented a translation model based on SMT for English (EN) to Punjabi
|
| 565 |
+
(PA) with their own corpus containing 3844 names in both languages with
|
| 566 |
+
BLEU and word accuracy as 0.4123 (with range 0-1) and 50.22%, respec-
|
| 567 |
+
tively.
|
| 568 |
+
(Nalluri et al (2011)) has created “enTel,” an SMT-based EN to Telugu(TE)
|
| 569 |
+
MT system, using the Johns Hopkins University Open Source Architecture (Li
|
| 570 |
+
et al (2009)). For the purpose of training the translation system, TE par- allel
|
| 571 |
+
dataset from the Enabling Minority Language Engineering (EMILLE) is
|
| 572 |
+
used for their work.
|
| 573 |
+
In the year 2014, an SMT Framework for Sinhala(SI)-Tamil(TA) MT Sys-
|
| 574 |
+
tem has been created by (Randil et al (2014)). In their work, the result
|
| 575 |
+
of SMT-dependent translation between language pairs, including TA-SI and
|
| 576 |
+
SI-TA has been shown. Outcomes of the experiments using the SMT model
|
| 577 |
+
give more noticeable results for the SI-TA than the TA-SI language pair. For
|
| 578 |
+
languages closely related, SMT shows remarkable results.
|
| 579 |
+
In 2017, a survey has been conducted by (Khan et al (2017)) on the IL-EN
|
| 580 |
+
language MT models reveal the importance of SMT over 8 languages i.e.
|
| 581 |
+
Hindi (HI), Bengali (BN), Gujarati (GU), Urdu (UR), Telugu (TE), Pun-
|
| 582 |
+
jabi (PA), Tamil (TA), and Malayalam (ML). In their work, EMILLE corpus
|
| 583 |
+
(Nalluri et al (2011)) is used and Moses SMT model is preferred to make
|
| 584 |
+
the translation models, with out-of-vocabulary (OOV) words transliterated
|
| 585 |
+
to EN. In their work, the evaluation using BLEU, NIST and UNK counts as
|
| 586 |
+
metrics reveals the overall SMT performance as satisfactory (PA-EN and UR-
|
| 587 |
+
EN models as the best and the HI-EN and GU-EN models as the worst). An
|
| 588 |
+
EN-BN SMT system has been presented by (Islam et al (2010)). In their work,
|
| 589 |
+
to handle OOV (out-of-vocabulary) words, a transliteration module is
|
| 590 |
+
presented. In order to address the systematic grammatical distinctions be-
|
| 591 |
+
tween EN and BN, a preposition handling module has been added. BLEU,
|
| 592 |
+
NIST and TER scores has been used to check the effectiveness of their sys-
|
| 593 |
+
|
| 594 |
+
13
|
| 595 |
+
|
| 596 |
+
|
| 597 |
+
|
| 598 |
+
|
| 599 |
+
|
| 600 |
+
tem.
|
| 601 |
+
Nowadays, NMT is widely appreciated for its advancement in the develop-
|
| 602 |
+
ment of machine translation with remarkable improvement in quality. Hence,
|
| 603 |
+
many researchers have compared both techniques for low and high-resource
|
| 604 |
+
languages.
|
| 605 |
+
(Antonio et al (2017)) has performed a thorough evaluation using statistical-
|
| 606 |
+
based and neural machine translation systems for nine language directions
|
| 607 |
+
along a variety of dimensions. In their experiment, for long sentences, SMT
|
| 608 |
+
systems perform better than the NMT. Recently, (Castilho et al (2017)) has
|
| 609 |
+
used automatic metrics and expert translators to conduct a thorough quan-
|
| 610 |
+
titative and qualitative comparison of NMT and SMT. SMT shows better
|
| 611 |
+
according to their experiments.
|
| 612 |
+
The comparison of NMT and SMT for the Nepali (NE) using the Nepali
|
| 613 |
+
National Corpus (NNC) with 6535 sentences has been shown by (Acharya et al
|
| 614 |
+
(2018)). The researchers have proved in their experiments that the SMT model
|
| 615 |
+
performs better than the NMT-based system with a small corpus with a 5.27
|
| 616 |
+
BLEU score.
|
| 617 |
+
In 2021, Long Short-Term Memory networks (LSTMs) integrated with atten-
|
| 618 |
+
tion mechanism using WAT corpus have been used in experiments by (Singh
|
| 619 |
+
et al (2003)) to achieve a 15.7 BLEU score as opposed to a baseline of 14.5
|
| 620 |
+
BLEU score.
|
| 621 |
+
(Abujar et al (2021)) has developed a BN-EN MT model on AmaderCAT cor-
|
| 622 |
+
pus using Sequence-to-Sequence (seq2seq) architecture, a special class of Re-
|
| 623 |
+
current Neural Networks to develop the translation system and has achieved
|
| 624 |
+
a BLEU score of 22.3.
|
| 625 |
+
In the year 2021, translation of English and Hindi-to-Tamil languages us- ing
|
| 626 |
+
both SMT and NMT has been presented by (Akshai et al (2021)). The
|
| 627 |
+
disadvantages of NMT have been shown in their experiments such as the
|
| 628 |
+
occurrence of numerous errors by NMT when interpreting domain terms and
|
| 629 |
+
OOV (Out of vocabulary) phrases. NMT frequently constructs inaccurate
|
| 630 |
+
lexical choices for polysemous words and occasionally counters reordering
|
| 631 |
+
mistakes while translating words and domain terms. The translations that
|
| 632 |
+
have been generated by the NMT models mostly include repetitions of pre-
|
| 633 |
+
viously transcribed words, odd translations, and many unexpected sentences
|
| 634 |
+
having no correlation with the original sentence.
|
| 635 |
+
|
| 636 |
+
14
|
| 637 |
+
|
| 638 |
+
|
| 639 |
+
|
| 640 |
+
|
| 641 |
+
3 Experimental Framework
|
| 642 |
+
3.1 Dataset
|
| 643 |
+
Samanantar and OPUS datasets for model building and standard benchmark
|
| 644 |
+
dataset i.e. Flores 200 for testing are utilized. Samanantar is the largest cor-
|
| 645 |
+
pus collection for ILs (Gowtham et al (2022)). The collection includes more
|
| 646 |
+
than 45 million sentence pairs in English and 11 ILs. The Samanantar Corpus
|
| 647 |
+
has been used for Assamese (AS), Malayalam (ML), Bengali (BN), Marathi
|
| 648 |
+
(MR), Gujarati (GU), Kannada (KN), Hindi (HI), Oriya (OR), Punjabi (PA),
|
| 649 |
+
Telugu (TE), and Tamil (TA) for the experiments. OPUS is a large resource
|
| 650 |
+
with freely available parallel corpora. The corpus includes data from many
|
| 651 |
+
domains and covers over 90 languages (Tiedemann (2012)). The OPUS cor-
|
| 652 |
+
pus is used for Sinhala (SI), Sindhi (SD), Urdu (UR), and Nepali (NE). Table 2
|
| 653 |
+
gives statistics of the dataset used in our experiments.
|
| 654 |
+
FLORES-200 (Marta et al (2022)) dataset is a multilingual parallel dataset
|
| 655 |
+
with 200 languages, that are used as human-translated benchmarks. It con-
|
| 656 |
+
sists of two corpora, labeled “dev” (997 lines) and “devtest” (1013 lines).
|
| 657 |
+
The “dev” dataset has been used for fine-tuning, and the “devtest” dataset
|
| 658 |
+
has been used for testing.
|
| 659 |
+
|
| 660 |
+
3.2 Methodology
|
| 661 |
+
Our proposed process comprises of following major steps:
|
| 662 |
+
1. Setting up SMT System Moses SMT Toolkit is used to build our
|
| 663 |
+
SMT systems. It is written in C++ and Perl. At the moment, this is
|
| 664 |
+
one of the best SMT tools available. First, Moses, GIZA++ (Och
|
| 665 |
+
(2003)), CMPH (for binarization) and SRILM in Ubuntu are installed.
|
| 666 |
+
For training, fine-tuning and testing processes, the system needs a par-
|
| 667 |
+
allel corpus of the language pair in addition to configurable phases
|
| 668 |
+
according to developer’s choice to follow.
|
| 669 |
+
2. Data Preprocessing A qualitative corpus plays a major role in any MT
|
| 670 |
+
task. While obtaining corpora from various sources, data qual- ity i.e.
|
| 671 |
+
critical for the effectiveness of an MT system, can never be
|
| 672 |
+
ascertained. So, removing unnecessary noise is an important task be-
|
| 673 |
+
fore using the data to train our statistical machine translation model.
|
| 674 |
+
Following processes are used to preprocess and clean it:
|
| 675 |
+
|
| 676 |
+
15
|
| 677 |
+
|
| 678 |
+
|
| 679 |
+
|
| 680 |
+
|
| 681 |
+
|
| 682 |
+
Table 2: Parallel corpus statistics
|
| 683 |
+
English to Indic
|
| 684 |
+
Parallel Corpus(Sentences)
|
| 685 |
+
Assamese (AS)
|
| 686 |
+
|
| 687 |
+
0.14M
|
| 688 |
+
Malayalam (ML)
|
| 689 |
+
5.85M
|
| 690 |
+
Bengali(BN)
|
| 691 |
+
8.52M
|
| 692 |
+
Marathi(MR)
|
| 693 |
+
3.32M
|
| 694 |
+
Gujarati(GU)
|
| 695 |
+
3.05M
|
| 696 |
+
Kannada(KN)
|
| 697 |
+
4.07M
|
| 698 |
+
Hindi(HI)
|
| 699 |
+
8.56M
|
| 700 |
+
Oriya(OR)
|
| 701 |
+
1.00M
|
| 702 |
+
Punjabi(PA)
|
| 703 |
+
2.42M
|
| 704 |
+
Telugu(TE)
|
| 705 |
+
4.82M
|
| 706 |
+
Sindhi(SD)
|
| 707 |
+
1.95M
|
| 708 |
+
Sinhala(SI)
|
| 709 |
+
8.68M
|
| 710 |
+
Nepali(NE)
|
| 711 |
+
3.35M
|
| 712 |
+
Tamil(TA)
|
| 713 |
+
5.16M
|
| 714 |
+
Urdu(UR)
|
| 715 |
+
8.95M
|
| 716 |
+
|
| 717 |
+
• Data Cleaning and Formatting The goal of data cleaning is
|
| 718 |
+
either to find and fix or to delete erroneous data from the corpus.
|
| 719 |
+
Here, characters those are used neither in ILs nor in English are
|
| 720 |
+
removed. Some of the punctuation in extended Unicode is con-
|
| 721 |
+
verted to its standard counterpart. Numbers in the IL corpus are
|
| 722 |
+
converted from English to IL scripts. Characters outside the stan-
|
| 723 |
+
dard alphabets of the language pair, extra spaces, and unprintable
|
| 724 |
+
characters are also removed from the corpus. The preprocessing
|
| 725 |
+
techniques used in our work have been summarized as follows:
|
| 726 |
+
– Removing unprintable characters
|
| 727 |
+
– Removing characters outside the language pair
|
| 728 |
+
– Removing extra spaces
|
| 729 |
+
– Deaccenting accented characters
|
| 730 |
+
– Changing non-standard Unicode punctuation characters in
|
| 731 |
+
both corpora to their standard counterparts
|
| 732 |
+
– Changing uncommon punctuations to more common ones
|
| 733 |
+
– Changing numbers to a uniform numbering system and script
|
| 734 |
+
|
| 735 |
+
16
|
| 736 |
+
|
| 737 |
+
|
| 738 |
+
|
| 739 |
+
|
| 740 |
+
|
| 741 |
+
3. Tokenization: It is the process of dividing a character sequence into
|
| 742 |
+
smaller units known as tokens based on a given character sequence and
|
| 743 |
+
a specified document unit. Words, punctuation, and numerals serve as
|
| 744 |
+
these tokens in our instance. The corpus is tokenized using a modified
|
| 745 |
+
Moses tokenizer (Koehn et al (2007)). Redundant punctuations (quo-
|
| 746 |
+
tation marks, apostrophes, and commas) are also removed from the
|
| 747 |
+
corpus.
|
| 748 |
+
4. Training Truecasing Model: This is the procedure for adding case
|
| 749 |
+
information to text that has been incorrectly cased or is not cased (Lita
|
| 750 |
+
et al (2003)). Data sparsity is lessened with the use of true casing. A
|
| 751 |
+
truecaser model (a model which changes the words at the beginning
|
| 752 |
+
of the sentence to the most common casing) is trained on the training
|
| 753 |
+
dataset. The Moses truecasing is used for the same.
|
| 754 |
+
5. Training Language and Translation Models: In MOSES, the
|
| 755 |
+
training procedure utilizes word and segment occurrences to draw con-
|
| 756 |
+
nections between the target and source languages. The language and
|
| 757 |
+
translation models are trained on the training dataset and binarized.
|
| 758 |
+
GIZA++ grow-diag-final-and alignment is used for word alignments,
|
| 759 |
+
which start with the intersection of the two alignments and then add
|
| 760 |
+
the additional alignment points.
|
| 761 |
+
The grow-diag-final-and model starts with the intersection of the align-
|
| 762 |
+
ments from source to target and target to source, then two steps are
|
| 763 |
+
used to add additional alignment points (Och (2003)):
|
| 764 |
+
grow-diag: For every neighboring point to the alignments measured,
|
| 765 |
+
if either source or target word is not aligned already but is present
|
| 766 |
+
in the union of the alignment, then the neighboring point is in-
|
| 767 |
+
cluded in the alignment.
|
| 768 |
+
final: If any phrase pairs are unaligned but present in the union, add
|
| 769 |
+
the point to the alignment.
|
| 770 |
+
• Word Alignment Model: After preprocessing the words, the
|
| 771 |
+
next step is word alignment. The proposed work employs the
|
| 772 |
+
GIZA++ (Och (2003)) incorporation of the IBM models to ac-
|
| 773 |
+
complish the word procedure. The GIZA++ model assesses the
|
| 774 |
+
likelihood of word-to-word alignment for each source and target
|
| 775 |
+
word in each sentence. To produce a good-quality word alignment,
|
| 776 |
+
|
| 777 |
+
17
|
| 778 |
+
|
| 779 |
+
−
|
| 780 |
+
−
|
| 781 |
+
−
|
| 782 |
+
−
|
| 783 |
+
|
| 784 |
+
|
| 785 |
+
|
| 786 |
+
|
| 787 |
+
the alignment is produced using a series of successive estimations.
|
| 788 |
+
To process a corpus with a larger quantity of sentences, the process
|
| 789 |
+
takes several hours. The alignment method’s outcomes establish
|
| 790 |
+
a connection between the target and source words.
|
| 791 |
+
• Reordering It is the process of restructuring the word order of
|
| 792 |
+
one natural language sentence to make it more similar to the word
|
| 793 |
+
order of another natural language sentence. It is a critical task
|
| 794 |
+
in transcription for languages with different syntactic structures.
|
| 795 |
+
The Moses system learns different reordering possibilities for each
|
| 796 |
+
phrase during the training process. Instead of default reordering,
|
| 797 |
+
the model uses the distance reordering model (Kumawat et al
|
| 798 |
+
(2014)).
|
| 799 |
+
– Distance-Based Reordering: The reordering of the tar- get
|
| 800 |
+
output phrases is represented by the relative distortion
|
| 801 |
+
probability distribution re (St, Et 1). Here, St refers to the
|
| 802 |
+
starting position of the source phrase that is interpreted into
|
| 803 |
+
the t 1 th target phrase. The reordering distance (St - Et
|
| 804 |
+
1) is calculated as follows: When taking source words out of
|
| 805 |
+
sequence, the reordering distance is the number of words ig-
|
| 806 |
+
nored (either forward or backward). If two phrases are trans-
|
| 807 |
+
lated in sequence, then t = Et 1 +1; that is, the first word of
|
| 808 |
+
the phrase immediately follows the last word of the pre-
|
| 809 |
+
vious phrase. A reordering cost of re(0) is used in this case.
|
| 810 |
+
The distance-based model assigns a linear cost to reordering
|
| 811 |
+
distance, implying that the movement of phrases over long
|
| 812 |
+
distances is more expensive.
|
| 813 |
+
6. Fine tuning: It is the process of determining the best configuration file
|
| 814 |
+
settings for a translation model when it is used for a specific pur- pose.
|
| 815 |
+
It uses a translation model to translate all 15 ILs source language phrases
|
| 816 |
+
in the tuning set. Then, it compares the model’s output to a set of
|
| 817 |
+
reference (human translations) and adjusts the settings to improve
|
| 818 |
+
translation quality. This procedure is repeated several times. The
|
| 819 |
+
tuning process repeats the steps with each iteration until the transla-
|
| 820 |
+
tion quality is optimized. The model is fine-tuned on the preprocessed
|
| 821 |
+
Flores-200 dev dataset.
|
| 822 |
+
7. Translation: The final model is used to translate the preprocessed
|
| 823 |
+
|
| 824 |
+
18
|
| 825 |
+
|
| 826 |
+
|
| 827 |
+
|
| 828 |
+
|
| 829 |
+
|
| 830 |
+
Flores-200 devtest dataset from the source to the target language.
|
| 831 |
+
8. Postprocessing and Detokenization: Redundant punctuation marks
|
| 832 |
+
(quotation marks, apostrophes, and commas) are removed, and the
|
| 833 |
+
translation file is detokenized using the Moses detokenizer.
|
| 834 |
+
9. Evaluation: The evaluation metrics use for our experiments are ME-
|
| 835 |
+
TEOR (Banerjee et al (2005)), RIBES (Wołk et al (2016)), and BLEU
|
| 836 |
+
(Papineni et al (2002)).
|
| 837 |
+
|
| 838 |
+
4 Essential metrics for MT translation evalu-
|
| 839 |
+
ation
|
| 840 |
+
The most crucial phase of any MT system is MT evaluation. Both automatic
|
| 841 |
+
and manual methods can be applied to analyze MT tasks. The effective-
|
| 842 |
+
ness of a system’s output can be evaluated either directly through human
|
| 843 |
+
assessments, or indirectly using reading cases, other downstream activities,
|
| 844 |
+
and even through estimating the amount of effort necessary to rectify the
|
| 845 |
+
output. A better outcome is obtained through manual evaluation, which
|
| 846 |
+
includes task-based evaluations, fluency and adequacy scores, human vot- ing
|
| 847 |
+
for translations task, post-editing measures, etc. However, the major
|
| 848 |
+
challenges of manual evaluation are time-intensiveness, absence of repeata-
|
| 849 |
+
bility and high cost. In order to evaluate the effectiveness of MT output,
|
| 850 |
+
different automated approaches are there such as Metric for Evaluation of
|
| 851 |
+
Translation with Explicit Ordering (METEOR), Bilingual Evaluation Un-
|
| 852 |
+
derstudy(BLEU), Levenshtein, Rank-based Intuitive Bilingual Evaluation
|
| 853 |
+
Score(RIBES), Word Error Rate (WER) and NIST exist. Several intuitive
|
| 854 |
+
advantages exist for automated metrics that can give points for synonyms or
|
| 855 |
+
paraphrases. A few of the evaluation metrics which are used in our work are
|
| 856 |
+
discussed below
|
| 857 |
+
1. Bilingual Evaluation Understudy (BLEU): The most widely used
|
| 858 |
+
method for evaluating machine translation (MT) is known as BLEU.
|
| 859 |
+
This method, first introduced in 2002 (Papineni et al (2002)) exam- ines
|
| 860 |
+
one or more reference translations to the hypothetical translation. When
|
| 861 |
+
the hypothetical translation matches numerous strings with the
|
| 862 |
+
reference translation, the MT evaluation gives it a higher score. The
|
| 863 |
+
BLEU system assigns a translation a score from 0 to 1. However, it is
|
| 864 |
+
|
| 865 |
+
|
| 866 |
+
19
|
| 867 |
+
|
| 868 |
+
1
|
| 869 |
+
|
| 870 |
+
|
| 871 |
+
|
| 872 |
+
usually represented as a percentage value. The nearer the translation is
|
| 873 |
+
to 1, the more it corresponds to the reference translation. This match-
|
| 874 |
+
ing of translation is conducted word-by-word in the same word order
|
| 875 |
+
in both datasets. SacreBLEU is used to calculate the BLEU scores of
|
| 876 |
+
baseline models.
|
| 877 |
+
2. Rank-based Intuitive Bilingual Evaluation Score (RIBES): It
|
| 878 |
+
is calculated by incorporating a rank correlation coefficient before uni-
|
| 879 |
+
gram matches, eliminating the necessity for higher-order n-gram matches.
|
| 880 |
+
This metric is concerned with word order. To compare SMT and ref-
|
| 881 |
+
erence translations, it employs Kendall’s tau coefficient (τ ) based on
|
| 882 |
+
word order to indicate rank differences (Wołk et al (2016)). To assure
|
| 883 |
+
positive values, the coefficient is normalized as shown below:
|
| 884 |
+
|
| 885 |
+
|
| 886 |
+
Normalized Kendall’s τ (NKT) = τ + 1
|
| 887 |
+
2
|
| 888 |
+
(5)
|
| 889 |
+
This coefficient can be paired with unigram-precision p1 and Brevity
|
| 890 |
+
Penalty BP and changed to prevent overestimation of the correlation
|
| 891 |
+
between only relevant words in SMT and reference translations.
|
| 892 |
+
|
| 893 |
+
|
| 894 |
+
RIBES = NKT.(pα).(BPβ )
|
| 895 |
+
(6)
|
| 896 |
+
Here, α and β are parameters between 0 and 1.
|
| 897 |
+
|
| 898 |
+
20
|
| 899 |
+
|
| 900 |
+
|
| 901 |
+
|
| 902 |
+
|
| 903 |
+
|
| 904 |
+
3. Metric for Evaluation of Translation with Explicit Ordering
|
| 905 |
+
(METEOR): Meteor scores a translation depending on explicit word-
|
| 906 |
+
by-word similarities between both the translation and a provided ref-
|
| 907 |
+
erence translation (Banerjee et al (2005)). It is specifically created to
|
| 908 |
+
generate sentence-level scores that are highly correlated with human
|
| 909 |
+
evaluations of translation quality. Meteor utilizes and highlights recall
|
| 910 |
+
in combination with precision, a feature that numerous measures have
|
| 911 |
+
verified as crucial for a strong correlation with human judgments. It also
|
| 912 |
+
intends to address the problem of imprecise reference translations by
|
| 913 |
+
utilizing adaptable word matching in consideration with synonyms and
|
| 914 |
+
morphological variances. To achieve a score of 1, the words of the
|
| 915 |
+
machine-generated output should be present in the reference and each
|
| 916 |
+
of the words of the reference is in the machine-generated output.
|
| 917 |
+
|
| 918 |
+
5 Results and Discussion
|
| 919 |
+
In this work, the evaluation metrics used are METEOR (Banerjee et al
|
| 920 |
+
(2005)), RIBES (Wołk et al (2016)), and BLEU (Papineni et al (2002)). All
|
| 921 |
+
the evaluation metrics used in our work are prominent metrics for deter-
|
| 922 |
+
mining the quality of the machine-translated text.
|
| 923 |
+
Table 3 displays the translation of all the 15 ILs to English and vice versa
|
| 924 |
+
using SMT without fine-tuning. Evaluation metrics of SMT with finetuning
|
| 925 |
+
using the Flores-200 dev dataset are shown in Table 4. RIBES and METEOR
|
| 926 |
+
range is 0-1. For EN-IL and IL-EN language using SMT, the BLEU score
|
| 927 |
+
lies between 0.46 to 13.09 and 0.49 to 15.41 respectively. The RIBES score for
|
| 928 |
+
EN-IL and IL-EN is between 0.04 to 0.63 and 0.14 to 0.61 respectively.
|
| 929 |
+
METEOR scores lie between 0.01 to 0.28 for EN-IL and 0.02 to 0.28 for
|
| 930 |
+
IL-EN. SMT models using distance reordering techniques are giving better
|
| 931 |
+
BLEU Scores for languages BN, PA, UR, HI, and GU than the rest. With-
|
| 932 |
+
out fine-tuning, SI performs the worst in terms of all three metrics of all
|
| 933 |
+
languages in both directions, whereas with fine-tuning EN-SI and TA-EN
|
| 934 |
+
perform worse than all other EN-IL and IL-EN models respectively with all
|
| 935 |
+
|
| 936 |
+
21
|
| 937 |
+
|
| 938 |
+
|
| 939 |
+
|
| 940 |
+
|
| 941 |
+
|
| 942 |
+
|
| 943 |
+
|
| 944 |
+
|
| 945 |
+
|
| 946 |
+
|
| 947 |
+
|
| 948 |
+
|
| 949 |
+
|
| 950 |
+
|
| 951 |
+
Table 3: Evaluation Metrics Result of SMT without Finetuning
|
| 952 |
+
|
| 953 |
+
Languages
|
| 954 |
+
Pairs
|
| 955 |
+
BLEU
|
| 956 |
+
RIBES
|
| 957 |
+
METEOR
|
| 958 |
+
AS
|
| 959 |
+
EN-AS
|
| 960 |
+
1.90
|
| 961 |
+
0.50
|
| 962 |
+
0.09
|
| 963 |
+
AS-EN
|
| 964 |
+
3.21
|
| 965 |
+
0.46
|
| 966 |
+
0.11
|
| 967 |
+
ML
|
| 968 |
+
EN-ML
|
| 969 |
+
3.79
|
| 970 |
+
0.27
|
| 971 |
+
0.08
|
| 972 |
+
ML-EN
|
| 973 |
+
4.59
|
| 974 |
+
0.43
|
| 975 |
+
0.12
|
| 976 |
+
BN
|
| 977 |
+
EN-BN
|
| 978 |
+
6.41
|
| 979 |
+
0.62
|
| 980 |
+
0.17
|
| 981 |
+
BN-EN
|
| 982 |
+
3.06
|
| 983 |
+
0.45
|
| 984 |
+
012
|
| 985 |
+
MR
|
| 986 |
+
EN-MR
|
| 987 |
+
3.17
|
| 988 |
+
0.43
|
| 989 |
+
0.09
|
| 990 |
+
MR-EN
|
| 991 |
+
3.62
|
| 992 |
+
0.43
|
| 993 |
+
0.09
|
| 994 |
+
GU
|
| 995 |
+
EN-GU
|
| 996 |
+
7.62
|
| 997 |
+
0.56
|
| 998 |
+
0.16
|
| 999 |
+
GU-EN
|
| 1000 |
+
10.14
|
| 1001 |
+
0.59
|
| 1002 |
+
0.21
|
| 1003 |
+
KN
|
| 1004 |
+
EN-KN
|
| 1005 |
+
5.06
|
| 1006 |
+
0.40
|
| 1007 |
+
0.11
|
| 1008 |
+
KN-EN
|
| 1009 |
+
7.17
|
| 1010 |
+
0.51
|
| 1011 |
+
0.16
|
| 1012 |
+
HI
|
| 1013 |
+
EN-HI
|
| 1014 |
+
13.09
|
| 1015 |
+
0.63
|
| 1016 |
+
0.28
|
| 1017 |
+
HI-EN
|
| 1018 |
+
15.41
|
| 1019 |
+
0.64
|
| 1020 |
+
0.28
|
| 1021 |
+
OR
|
| 1022 |
+
EN-OR
|
| 1023 |
+
3.92
|
| 1024 |
+
0.59
|
| 1025 |
+
0.14
|
| 1026 |
+
OR-EN
|
| 1027 |
+
6.41
|
| 1028 |
+
0.52
|
| 1029 |
+
0.17
|
| 1030 |
+
PA
|
| 1031 |
+
EN-PA
|
| 1032 |
+
7.22
|
| 1033 |
+
0.63
|
| 1034 |
+
0.18
|
| 1035 |
+
PA-EN
|
| 1036 |
+
11.7
|
| 1037 |
+
0.61
|
| 1038 |
+
0.24
|
| 1039 |
+
TE
|
| 1040 |
+
EN-TE
|
| 1041 |
+
8.16
|
| 1042 |
+
0.42
|
| 1043 |
+
0.12
|
| 1044 |
+
TE-EN
|
| 1045 |
+
5.77
|
| 1046 |
+
0.52
|
| 1047 |
+
0.18
|
| 1048 |
+
SD
|
| 1049 |
+
EN-SD
|
| 1050 |
+
1.29
|
| 1051 |
+
0.39
|
| 1052 |
+
0.08
|
| 1053 |
+
SD-EN
|
| 1054 |
+
2.48
|
| 1055 |
+
0.35
|
| 1056 |
+
0.09
|
| 1057 |
+
SI
|
| 1058 |
+
EN-SI
|
| 1059 |
+
0.93
|
| 1060 |
+
0.05
|
| 1061 |
+
0.02
|
| 1062 |
+
SI-EN
|
| 1063 |
+
0.49
|
| 1064 |
+
0.14
|
| 1065 |
+
0.05
|
| 1066 |
+
NE
|
| 1067 |
+
EN-NE
|
| 1068 |
+
6.00
|
| 1069 |
+
0.58
|
| 1070 |
+
0.16
|
| 1071 |
+
NE-EN
|
| 1072 |
+
8.29
|
| 1073 |
+
0.53
|
| 1074 |
+
0.19
|
| 1075 |
+
TA
|
| 1076 |
+
EN-TA
|
| 1077 |
+
2.78
|
| 1078 |
+
0.16
|
| 1079 |
+
0.05
|
| 1080 |
+
TA-EN
|
| 1081 |
+
2.64
|
| 1082 |
+
0.31
|
| 1083 |
+
0.07
|
| 1084 |
+
UR
|
| 1085 |
+
EN-UR
|
| 1086 |
+
9.43
|
| 1087 |
+
0.62
|
| 1088 |
+
0.24
|
| 1089 |
+
UR-EN
|
| 1090 |
+
11.35
|
| 1091 |
+
0.61
|
| 1092 |
+
0.23
|
| 1093 |
+
|
| 1094 |
+
|
| 1095 |
+
22
|
| 1096 |
+
|
| 1097 |
+
|
| 1098 |
+
|
| 1099 |
+
|
| 1100 |
+
|
| 1101 |
+
|
| 1102 |
+
|
| 1103 |
+
|
| 1104 |
+
|
| 1105 |
+
|
| 1106 |
+
|
| 1107 |
+
|
| 1108 |
+
|
| 1109 |
+
|
| 1110 |
+
Table 4: Evaluation Metrics Result of SMT with Finetuning
|
| 1111 |
+
|
| 1112 |
+
Languages
|
| 1113 |
+
Pairs
|
| 1114 |
+
BLEU
|
| 1115 |
+
RIBES
|
| 1116 |
+
METEOR
|
| 1117 |
+
AS
|
| 1118 |
+
EN-AS
|
| 1119 |
+
2.17
|
| 1120 |
+
0.50
|
| 1121 |
+
0.08
|
| 1122 |
+
AS-EN
|
| 1123 |
+
3.21
|
| 1124 |
+
0.42
|
| 1125 |
+
0.10
|
| 1126 |
+
ML
|
| 1127 |
+
EN-ML
|
| 1128 |
+
2.05
|
| 1129 |
+
0.23
|
| 1130 |
+
0.06
|
| 1131 |
+
ML-EN
|
| 1132 |
+
1.84
|
| 1133 |
+
0.27
|
| 1134 |
+
0.06
|
| 1135 |
+
BN
|
| 1136 |
+
EN-BN
|
| 1137 |
+
8.26
|
| 1138 |
+
0.63
|
| 1139 |
+
0.19
|
| 1140 |
+
BN-EN
|
| 1141 |
+
12.16
|
| 1142 |
+
0.60
|
| 1143 |
+
0.23
|
| 1144 |
+
MR
|
| 1145 |
+
EN-MR
|
| 1146 |
+
2.43
|
| 1147 |
+
0.39
|
| 1148 |
+
0.08
|
| 1149 |
+
MR-EN
|
| 1150 |
+
2.49
|
| 1151 |
+
0.36
|
| 1152 |
+
0.07
|
| 1153 |
+
GU
|
| 1154 |
+
EN-GU
|
| 1155 |
+
5.82
|
| 1156 |
+
0.52
|
| 1157 |
+
0.14
|
| 1158 |
+
GU-EN
|
| 1159 |
+
3.56
|
| 1160 |
+
0.45
|
| 1161 |
+
0.01
|
| 1162 |
+
KN
|
| 1163 |
+
EN-KN
|
| 1164 |
+
3.35
|
| 1165 |
+
0.09
|
| 1166 |
+
0.14
|
| 1167 |
+
KN-EN
|
| 1168 |
+
3.67
|
| 1169 |
+
0.41
|
| 1170 |
+
0.10
|
| 1171 |
+
HI
|
| 1172 |
+
EN-HI
|
| 1173 |
+
8.64
|
| 1174 |
+
0.57
|
| 1175 |
+
0.22
|
| 1176 |
+
HI-EN
|
| 1177 |
+
5.38
|
| 1178 |
+
0.49
|
| 1179 |
+
0.14
|
| 1180 |
+
OR
|
| 1181 |
+
EN-OR
|
| 1182 |
+
5.25
|
| 1183 |
+
0.58
|
| 1184 |
+
0.15
|
| 1185 |
+
OR-EN
|
| 1186 |
+
2.22
|
| 1187 |
+
0.39
|
| 1188 |
+
0.11
|
| 1189 |
+
PA
|
| 1190 |
+
EN-PA
|
| 1191 |
+
5.71
|
| 1192 |
+
0.60
|
| 1193 |
+
0.15
|
| 1194 |
+
PA-EN
|
| 1195 |
+
7.75
|
| 1196 |
+
0.55
|
| 1197 |
+
0.19
|
| 1198 |
+
TE
|
| 1199 |
+
EN-TE
|
| 1200 |
+
4.4
|
| 1201 |
+
0.38
|
| 1202 |
+
0.10
|
| 1203 |
+
TE-EN
|
| 1204 |
+
3.34
|
| 1205 |
+
0.44
|
| 1206 |
+
0.12
|
| 1207 |
+
SD
|
| 1208 |
+
EN-SD
|
| 1209 |
+
1.59
|
| 1210 |
+
0.41
|
| 1211 |
+
0.09
|
| 1212 |
+
SD-EN
|
| 1213 |
+
2.53
|
| 1214 |
+
0.38
|
| 1215 |
+
0.09
|
| 1216 |
+
SI
|
| 1217 |
+
EN-SI
|
| 1218 |
+
0.46
|
| 1219 |
+
0.04
|
| 1220 |
+
0.01
|
| 1221 |
+
SI-EN
|
| 1222 |
+
3.11
|
| 1223 |
+
0.37
|
| 1224 |
+
0.11
|
| 1225 |
+
NE
|
| 1226 |
+
EN-NE
|
| 1227 |
+
4.00
|
| 1228 |
+
0.55
|
| 1229 |
+
0.14
|
| 1230 |
+
NE-EN
|
| 1231 |
+
5.25
|
| 1232 |
+
0.49
|
| 1233 |
+
0.13
|
| 1234 |
+
TA
|
| 1235 |
+
EN-TA
|
| 1236 |
+
1.86
|
| 1237 |
+
0.16
|
| 1238 |
+
0.05
|
| 1239 |
+
TA-EN
|
| 1240 |
+
1.03
|
| 1241 |
+
0.08
|
| 1242 |
+
0.02
|
| 1243 |
+
UR
|
| 1244 |
+
EN-UR
|
| 1245 |
+
6.34
|
| 1246 |
+
0.56
|
| 1247 |
+
0.19
|
| 1248 |
+
UR-EN
|
| 1249 |
+
7.07
|
| 1250 |
+
0.54
|
| 1251 |
+
0.18
|
| 1252 |
+
|
| 1253 |
+
23
|
| 1254 |
+
|
| 1255 |
+
|
| 1256 |
+
|
| 1257 |
+
three metrics. HI and BN languages have qualitative, large, and less noisy
|
| 1258 |
+
datasets compared to other languages. Hence, HI performs the best among all
|
| 1259 |
+
languages without fine-tuning in all three metrics in both directions, and BN
|
| 1260 |
+
performs the best among all languages with fine-tuning in both direc- tions
|
| 1261 |
+
with respect to BLEU and RIBES. In addition, UR and PA also produce good
|
| 1262 |
+
RIBES metrics than other languages. RIBES score for PA is 0.63(for EN-
|
| 1263 |
+
PA) and 0.61(PA-EN), and for UR, RIBES score is 0.62(EN-UR) and
|
| 1264 |
+
0.61(UR-EN).
|
| 1265 |
+
Even though SI has a good amount of corpus, the corpus does not have reli-
|
| 1266 |
+
able translations compared to other languages. For example, the sentence in
|
| 1267 |
+
English “Heb. 11:32-34; Judg. 16:18-21, 28-30 Jehovah’s spirit operated on
|
| 1268 |
+
Samson in a unique way because of unusual circumstances” has been trans-
|
| 1269 |
+
lated to Sinhala in the corpus as “11:32-34; Gනි.”, which only translates
|
| 1270 |
+
“Heb. 11:32-34;”. Hence, SI does not perform well compared to other lan-
|
| 1271 |
+
guages. Similarly, in the EN-TA corpus, the sentence “He’s my boss” has
|
| 1272 |
+
been translated to “அவர் எனது ே மலாளர் மட்டும்தான் .” which ac-
|
| 1273 |
+
tually means “He is only my manager”. From the example, it is clear that
|
| 1274 |
+
EN-TA corpus also has ambiguity. Additionally, even though the ILs-English
|
| 1275 |
+
and English-ILs systems are trained using the same corpus, a significant dis-
|
| 1276 |
+
crepancy in the BLEU scores is observed. This is due to the significant
|
| 1277 |
+
morphological diversity of ILs and the relative difficulty of translating from
|
| 1278 |
+
English to ILs. It has been observed that SI has a high number of lines (8.68
|
| 1279 |
+
M) but performs poorly as compared to languages like PA (2.42 M) and GU
|
| 1280 |
+
(3.05 M). It is also observed that languages with very steep slopes tend to
|
| 1281 |
+
have low scores. For example, EN-TA and EN-ML have 60% sentences with
|
| 1282 |
+
less than 4 tokens, and they have not-so-good scores as shown in Figure 1.
|
| 1283 |
+
In contrast, languages with good scores, like HI and BN have more gentle
|
| 1284 |
+
slopes. So, length of sentences is a contributing factor. EN-SD is an ex-
|
| 1285 |
+
ception which has a gentle slope but does not give good scores, because the
|
| 1286 |
+
corpus does not have good translation quality. Therefore, the quality of the
|
| 1287 |
+
corpus matters more than the size of the dataset.
|
| 1288 |
+
|
| 1289 |
+
6 Conclusion and Future Work
|
| 1290 |
+
This paper has presented the MT work for 15 ILs to English and vice versa
|
| 1291 |
+
using SMT. It also describes the linguistic features of all 15 ILs. A tailor-
|
| 1292 |
+
made preprocessing approach has been incorporated into this work. The
|
| 1293 |
+
|
| 1294 |
+
24
|
| 1295 |
+
|
| 1296 |
+
|
| 1297 |
+
|
| 1298 |
+
|
| 1299 |
+
|
| 1300 |
+
|
| 1301 |
+
|
| 1302 |
+
|
| 1303 |
+
|
| 1304 |
+
|
| 1305 |
+
|
| 1306 |
+
|
| 1307 |
+
|
| 1308 |
+
|
| 1309 |
+
|
| 1310 |
+
|
| 1311 |
+
|
| 1312 |
+
|
| 1313 |
+
Figure 1: Less than ogive for number of tokens in a sentence for all fifteen
|
| 1314 |
+
language corpora
|
| 1315 |
+
|
| 1316 |
+
LessthanOgiveforNumberoflokens
|
| 1317 |
+
1.2
|
| 1318 |
+
given
|
| 1319 |
+
numberoftokenslessthan
|
| 1320 |
+
1
|
| 1321 |
+
0.8
|
| 1322 |
+
0.6
|
| 1323 |
+
ofsentences
|
| 1324 |
+
0.4
|
| 1325 |
+
Ratio
|
| 1326 |
+
0.2
|
| 1327 |
+
0
|
| 1328 |
+
0
|
| 1329 |
+
1
|
| 1330 |
+
2
|
| 1331 |
+
m
|
| 1332 |
+
4
|
| 1333 |
+
5
|
| 1334 |
+
6
|
| 1335 |
+
7
|
| 1336 |
+
8
|
| 1337 |
+
9
|
| 1338 |
+
Numberoftokens
|
| 1339 |
+
EN-AS(AS)
|
| 1340 |
+
EN-SI(SI)
|
| 1341 |
+
EN-ML(ML)
|
| 1342 |
+
EN-MR(MR)
|
| 1343 |
+
EN-OR(OR)
|
| 1344 |
+
EN-SD(SD)
|
| 1345 |
+
EN-UR(UR)
|
| 1346 |
+
—EN-BN(BN)
|
| 1347 |
+
EN-GU(GU)
|
| 1348 |
+
EN-HI(HI)
|
| 1349 |
+
EN-KN(KN)
|
| 1350 |
+
EN-NE(NE)
|
| 1351 |
+
EN-PA(PA)
|
| 1352 |
+
EN-TA(TA)
|
| 1353 |
+
EN-TE(TE)25
|
| 1354 |
+
|
| 1355 |
+
|
| 1356 |
+
|
| 1357 |
+
|
| 1358 |
+
|
| 1359 |
+
model has utilized the grow-diag-final-and alignment model and distance re-
|
| 1360 |
+
ordering model. For checking the quality of translation, different evaluation
|
| 1361 |
+
Metrics such as BLEU, RIBES, and METEOR are utilized in this work.
|
| 1362 |
+
From the result, it is observed that the proposed SMT model is quite satis-
|
| 1363 |
+
factory for some of the ILs. However, the level of performance is not at par
|
| 1364 |
+
with the rest of the ILs and there lies the need of improvement to be made.
|
| 1365 |
+
Due to the scarcity and quality of parallel corpus, the metrics obtained are
|
| 1366 |
+
quite low.
|
| 1367 |
+
It has been observed that the translations of some of the languages are not
|
| 1368 |
+
sufficiently accurate. Measures of validating corpus quality shall be explored
|
| 1369 |
+
in order to observe the corpus quality and remove inaccurate lines. Dravid- ian
|
| 1370 |
+
languages are in general agglutinative languages (words are made up of
|
| 1371 |
+
morphemes, with each morpheme contributing to the meaning of the word).
|
| 1372 |
+
In future, means to infer translations from the breakdown of words in these
|
| 1373 |
+
languages shall also be explored.
|
| 1374 |
+
Interestingly, in some of the ILs, finetuning schemes are hampering the qual-
|
| 1375 |
+
ity. The causes of this phenomenon shall be analyzed and mitigated via
|
| 1376 |
+
techniques such as noise reduction, corpus cleaning, and finetuning schemes
|
| 1377 |
+
for those languages to ensure better quality. In addition, more language
|
| 1378 |
+
pairs and corpora can be analyzed and evaluated using various other meth-
|
| 1379 |
+
ods. Other techniques, such as hybridized SMT-NMT systems and the usage
|
| 1380 |
+
of other alignment and reordering models will be studied for further course
|
| 1381 |
+
of research.
|
| 1382 |
+
|
| 1383 |
+
References
|
| 1384 |
+
Dorr, Bonnie J., Eduard H. Hovy, and Lori S. Levin. 2004. Natural Lan-
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|
| 1 |
+
arXiv:2301.01023v1 [physics.comp-ph] 3 Jan 2023
|
| 2 |
+
Performance investigation of supercapacitors
|
| 3 |
+
with PEO-based gel polymer & ionic liquid
|
| 4 |
+
electrolytes: Molecular Dynamics Simulation
|
| 5 |
+
Nasrin Eyvazi,† Davood Abbaszadeh,† Morad Biagooi,‡ and SeyedEhsan Nedaaee
|
| 6 |
+
Oskoee∗,†,¶
|
| 7 |
+
†Department of Physics, Institute for Advanced Studies in Basic Sciences (IASBS), Zanjan
|
| 8 |
+
45137-66731, Iran
|
| 9 |
+
‡Intelligent Data Aim Ltd (IDA Ltd), Science and Technology Park of Institute for
|
| 10 |
+
Advanced studies in Basic Sciences, Zanjan 45137-65697, Iran
|
| 11 |
+
¶Research Center for Basic Sciences & Modern Technologies (RBST), Institute for
|
| 12 |
+
Advanced Studies in Basic Sciences (IASBS), Zanjan 45137-66731, Iran
|
| 13 |
+
E-mail: nedaaee@iasbs.ac.ir
|
| 14 |
+
Phone: (+98) 241-415-2217. Fax: (+98) 241-415-2104
|
| 15 |
+
Abstract
|
| 16 |
+
Due to the importance of using supercapacitors in electronic storage devices, im-
|
| 17 |
+
proving their efficiency is one of the topics that has attracted the attention of many
|
| 18 |
+
researchers. Choosing the proper electrolyte for supercapacitors is one of the most sig-
|
| 19 |
+
nificant factors affecting the performance of supercapacitors. In this paper, two classes
|
| 20 |
+
of electrolytes, i.e.
|
| 21 |
+
liquid electrolyte (ionic liquid electrolyte) and solid electrolyte
|
| 22 |
+
(polymer electrolyte) are compared by molecular dynamics simulation. We consider
|
| 23 |
+
the polymer electrolyte in linear and network configurations. The results show that
|
| 24 |
+
1
|
| 25 |
+
|
| 26 |
+
although ionic liquid-based supercapacitors have a larger differential capacitance, since
|
| 27 |
+
they have a smaller operation voltage, the amount of energy stored is less than poly-
|
| 28 |
+
mer electrolyte-based supercapacitors. Also, our investigations indicate that polymer
|
| 29 |
+
electrolyte-based supercapacitors have more mechanical stability. Therefore, they can
|
| 30 |
+
be considered a very suitable alternative to liquid electrolyte-based supercapacitors that
|
| 31 |
+
do not have known liquid electrolyte problems and display better performance.
|
| 32 |
+
Introduction
|
| 33 |
+
Supercapacitors (SCs), also known as Electric Double Layer Capacitors (EDLCs), have re-
|
| 34 |
+
cently attracted much attention in the field of electrical energy storage. The SCs fill the gap
|
| 35 |
+
between batteries and conventional capacitors in terms of energy and power density. They
|
| 36 |
+
consist of two porous electrodes immersed in an electrolyte. Due to the potential differ-
|
| 37 |
+
ence between the electrodes, the charged electrodes repel the co-ions in the electrolyte while
|
| 38 |
+
attracting their counter-ions, resulting in charge separation and charge storage.
|
| 39 |
+
The SCs have higher energy density in comparison with conventional capacitors due
|
| 40 |
+
to their porous electrodes with large surface areas and small charge separation distances.1
|
| 41 |
+
Also, compared to batteries, SCs have the advantages of higher power density induced by
|
| 42 |
+
a fast charging/discharging rate (in seconds), a long cycle life (4,100,000 cycles), and high
|
| 43 |
+
power density.1 Despite their higher power density, they cannot store the same amount of
|
| 44 |
+
energy as batteries.1 Extensive efforts and research have been devoted to increasing the
|
| 45 |
+
energy density of SCs to 20-30 Wh/L to solve the problems and satisfy the performance
|
| 46 |
+
demands.2–4 According to relation E = 1
|
| 47 |
+
2CV 2, the energy density (E) of SCs is proportional
|
| 48 |
+
to the capacitance (C) and the square of the voltage (V ). Therefore, increasing either the
|
| 49 |
+
capacitance or the voltage of a cell can be an effective way to achieve high energy density.2
|
| 50 |
+
The efficiency of SCs depends mainly on both electrolyte and electrode structure. The
|
| 51 |
+
pore size and surface area of electrodes, ionic conductivity, and electrolyte operating voltage
|
| 52 |
+
window play a significant role in developing high-performance and flexible SCs.5 Especially
|
| 53 |
+
2
|
| 54 |
+
|
| 55 |
+
in the case of liquid electrolytes, they have some disadvantages for use in flexible SCs like
|
| 56 |
+
being toxic and corrosive,2 requiring high-cost packaging to fabricate, and are associated
|
| 57 |
+
with leakage problems.2,6 In general, the critical features of an ideal electrolyte include: (1)
|
| 58 |
+
a wide voltage and temperature window; (2) a high ionic conductivity; (3) a high chemical
|
| 59 |
+
and mechanical stability; (4) well-matched with the electrolyte materials; (5) low volatility
|
| 60 |
+
and flammability; (6) safety; and (7) simple processing with low cost.6–8
|
| 61 |
+
To overcome the limitations of liquid electrolytes, polymer electrolytes (PEs) were in-
|
| 62 |
+
troduced. In 1970, Armand first used PE in Lithium Ion Batteries (LIBs) and proposed
|
| 63 |
+
LIBs with improved efficiency and energy density.9 PEs consist of a macromolecule matrix
|
| 64 |
+
dissolved in a low viscosity and high dielectric constant organic solvent.9 PEs have many
|
| 65 |
+
advantages such as avoiding liquid leakage and corrosion problems, good ionic conductivity,
|
| 66 |
+
high chemical and mechanical stability, high energy density, safety, solvent-free condition,
|
| 67 |
+
being light in weight, low cost, and simple manufacturing process.6–9
|
| 68 |
+
Due to the advantages of PEs, they are ideal candidates for use in SCs as electrolytes.
|
| 69 |
+
PEs for SCs can be classified into three categories: (1) solid polymer electrolytes (SPEs),
|
| 70 |
+
(2) gel polymer electrolytes (GPEs), and (3) polyelectrolytes. The SPE is composed of a
|
| 71 |
+
polymer (e.g., PEO) and a salt (e.g., LiCl), without any solvents. The ions in the SPE are
|
| 72 |
+
transported through the polymer2,5 and the polymer works as a host matrix for ion move-
|
| 73 |
+
ment.2,10 In contrast, the GPE consists of a polymer host (e.g., PVA) and a liquid electrolyte
|
| 74 |
+
or a conducting salt dissolved in a solvent.2,11 The polymer in GPE is swollen by the solvent
|
| 75 |
+
and acts as a dynamic moving matrix. The conductivity of ions occurs through the solvent
|
| 76 |
+
instead of the polymer phase.2,11 In GPEs, the liquid electrolyte generally provides free ions
|
| 77 |
+
that participate in conductivity enhancement and also acts as a conductive medium. In
|
| 78 |
+
addition, the polymer provides perfect mechanical stability by increasing the viscosity of
|
| 79 |
+
the electrolyte.5 Recently, researchers have shown that using Ionic Liquids (ILs) can im-
|
| 80 |
+
prove ionic conductivity and cell voltage, resulting to improvement in the electrochemical
|
| 81 |
+
performance of GPE.5 By its softening effect on the polymer chains, IL can increase the
|
| 82 |
+
3
|
| 83 |
+
|
| 84 |
+
electrolyte’s ionic conductivity and facilitate ion transfer.5 GPE based on ILs and linear
|
| 85 |
+
polymers usually exhibit poor mechanical properties, including both strength and flexibil-
|
| 86 |
+
ity, because of their few polymer chain entanglements separated by small molecules.12 To
|
| 87 |
+
generate polymer networks, cross-linking strategies have been proposed in recent years. The
|
| 88 |
+
behaviors and performance of polymer gels are largely determined by the structure of the
|
| 89 |
+
polymer network that makes up the gel. This is due to the interaction between the net-
|
| 90 |
+
work and the solvent.5 Gels generally have high mobility because the polymer networks are
|
| 91 |
+
dissolved by a large amount of entrapped solvent.5
|
| 92 |
+
In the polyelectrolyte, ionic conductivity is created by charged polymer chains.12 As
|
| 93 |
+
it turns out, each type of these solid-state electrolytes has its advantages and disadvan-
|
| 94 |
+
tages. Typically, GPEs have the highest ionic conductivity among the three types of solid-
|
| 95 |
+
state electrolytes.5,12 Due to the liquid phase in the GPE, its ionic conductivity is signif-
|
| 96 |
+
icantly higher than dry SPE. Therefore, GPE-based SCs currently dominate the products
|
| 97 |
+
of solid electrolyte-based SCs.
|
| 98 |
+
Several polymer matrices have been explored for prepar-
|
| 99 |
+
ing GPEs in the role of host polymer including: poly (vinyl alcohol) (PVA), poly (acrylic
|
| 100 |
+
acid) (PAA), potassium polyacrylate (PAAK), poly (ethyl oxide) (PEO), poly (methyl-
|
| 101 |
+
methacrylate) (PMMA), poly (ether ether ketone) (PEEK), and poly (vinylidene fluoride-
|
| 102 |
+
co-hexafluoro-propylene) (PVDF-HFP).2
|
| 103 |
+
Beyond all of the experimental achievements,6,13–16 modeling the EDLCs under differ-
|
| 104 |
+
ent physical conditions would provide a lot of insight into the system’s physics. Modeling
|
| 105 |
+
the microstructure will reveal how the related dynamics for charge carriers happen. So far,
|
| 106 |
+
numerous types of research have been done on liquid electrolyte-based SCs to explore the
|
| 107 |
+
performance of different kinds of liquid electrolyte-based SCs and the effect of electrode struc-
|
| 108 |
+
ture and its pore size.17–20 Our previous work,21 models the third classification of polymer
|
| 109 |
+
electrolytes (polyelectrolytes). In this work, considering the advantages of GPEs compared
|
| 110 |
+
to other polymer electrolytes and their useful applications, we investigated the behavior of
|
| 111 |
+
GPE-based SCs using the molecular dynamics simulation method. Here, we compared IL-
|
| 112 |
+
4
|
| 113 |
+
|
| 114 |
+
based and GPE-based SCs in order to find out the effects of adding host polymers to the
|
| 115 |
+
IL electrolyte. In the first section, we describe the method of simulation under different
|
| 116 |
+
conditions. Based on the results we get from our model, we discuss the pros and cons of
|
| 117 |
+
using GPEs and IL electrolytes in SCs.
|
| 118 |
+
Method
|
| 119 |
+
Systems’ model and force field parameters
|
| 120 |
+
Molecular Dynamics (MD) simulations have been widely used to describe the behavior of SCs.
|
| 121 |
+
Using MD simulations, we compared liquid electrolyte-based SCs with PE-based SCs under
|
| 122 |
+
various conditions. The simulations were carried out by the CAVIAR software package.22
|
| 123 |
+
We have investigated the performance of three different systems with similar electrodes but
|
| 124 |
+
different electrolytes. The electrolytes were confined between two electrodes with single slit-
|
| 125 |
+
pore geometry, placed at a distance of 15 nm from each other. This model called a slit-pore
|
| 126 |
+
model was introduced by Breitsprecher et al18,23 for simulating porous media.
|
| 127 |
+
The slit-pore length was set to 15 nm, in order to be compared with the bulk region and
|
| 128 |
+
the width of the pore is 2.5 nm (larger than the size of two ionic particles) so that at least
|
| 129 |
+
two ionic particles can pass through the pore.24
|
| 130 |
+
To compare the electrolyte role we have simulated the above mentioned pore structure
|
| 131 |
+
with different electrolyte systems; liquid electrolyte (system A), linear polymer electrolyte
|
| 132 |
+
(system B), and polymer network electrolyte (system C). By comparing the results, we can
|
| 133 |
+
discuss the effects and the function of different electrolytes.
|
| 134 |
+
System A: Liquid electrolyte-based supercapacitors
|
| 135 |
+
Our first model contains IL electrolytes confined between those described electrodes. We
|
| 136 |
+
used Coarse-Grained (CG) models of ILs, where ions are soft spheres with diameters dcation
|
| 137 |
+
= danion = 1 nm and valency q = ± 1, in units of the elementary charge. The mass of
|
| 138 |
+
5
|
| 139 |
+
|
| 140 |
+
cations and anions are mcation = 117.17 g
|
| 141 |
+
mol and manion = 86.81 g
|
| 142 |
+
mol corresponding to EMIM+
|
| 143 |
+
and BF4-.
|
| 144 |
+
All the particles interact with the non-bonding Lennard-Jones (LJ) potential:
|
| 145 |
+
VLJ(rij) =
|
| 146 |
+
|
| 147 |
+
|
| 148 |
+
|
| 149 |
+
|
| 150 |
+
|
| 151 |
+
4εij[( σij
|
| 152 |
+
rij )12 − ( σij
|
| 153 |
+
rij )6]
|
| 154 |
+
;
|
| 155 |
+
r ≤ rcut
|
| 156 |
+
0
|
| 157 |
+
;
|
| 158 |
+
r ≥ rcut
|
| 159 |
+
(1)
|
| 160 |
+
Where rij is the relative distance between each pair of particles, ε and σ are the length
|
| 161 |
+
and energy parameters. In calculating the LJ potential, rcut =
|
| 162 |
+
6√
|
| 163 |
+
2 σ is the cutoff length
|
| 164 |
+
to ensure short-range repulsive force at any distance. In addition, charged particles also
|
| 165 |
+
interact through the electrostatic non-bonding potential:
|
| 166 |
+
VC(rij) =
|
| 167 |
+
�
|
| 168 |
+
i
|
| 169 |
+
�
|
| 170 |
+
i<j
|
| 171 |
+
zizje2
|
| 172 |
+
4πǫ|ri − rj|
|
| 173 |
+
(2)
|
| 174 |
+
The ǫ and e are the electric permittivity and the electrical charge. The z = ±1 is the valency
|
| 175 |
+
of ions. For the electrostatic interactions we used the electric permittivity of ǫ = 10, a typical
|
| 176 |
+
value for ILs at 300 ◦K.17
|
| 177 |
+
System B: Linear polymer electrolyte-based supercapacitors
|
| 178 |
+
In system B, we added polymer hosts to system A to simulate GPE-based SCs. By com-
|
| 179 |
+
paring these two systems’ behavior, we can find out the advantages of one over another.
|
| 180 |
+
Poly(ethylene oxide) (PEO) with the formula H3C-O-(CH2-CH2-O)n-CH3,25 the most com-
|
| 181 |
+
mon polymer with a broad range of applications in polymer chemistry,26 biotechnology,27
|
| 182 |
+
and medical science,9,28 is used as a host polymer in our simulations. We used MARTINI-like
|
| 183 |
+
CG models for PEO simulation.25,28 Fig.1 represents the CG model for PEO2.
|
| 184 |
+
Generally, the MARTINI potential consists of bond, angle, LJ, electrostatic, and torsional
|
| 185 |
+
terms. In our system, two consecutive beads in each chain are connected by a harmonic
|
| 186 |
+
6
|
| 187 |
+
|
| 188 |
+
Figure 1: PEO2 and its CG model.
|
| 189 |
+
stretching spring whose potential is taken to be:
|
| 190 |
+
Vbond(r) = 1
|
| 191 |
+
2Kb(r − r0)2
|
| 192 |
+
(3)
|
| 193 |
+
Where Kb is the bond force constant, r is the instantaneous bond length, and r0 is the
|
| 194 |
+
equilibrium length of the bond. Bond angle is the angle formed between three atoms across
|
| 195 |
+
at least two bonds which can be described as:
|
| 196 |
+
Vangle(θ) = 1
|
| 197 |
+
2Kθ(cosθ − cosθ0)
|
| 198 |
+
(4)
|
| 199 |
+
and the torsion angle (also called dihedral angle) is defined by 3 consecutive bonds involving
|
| 200 |
+
4 atoms:
|
| 201 |
+
Vdihedral(φ) =
|
| 202 |
+
4
|
| 203 |
+
�
|
| 204 |
+
n=1
|
| 205 |
+
Kφ,n(1 + cos(nφ − φn))
|
| 206 |
+
(5)
|
| 207 |
+
Where n and φ are the multiplicities and offsets of the n individual dihedral terms. The
|
| 208 |
+
force constants for these bonded interactions are listed in Table.1.25
|
| 209 |
+
Table 1: Parameters for bonded interactions for modeling CG PEO.
|
| 210 |
+
Bond
|
| 211 |
+
Angle
|
| 212 |
+
Dihedral
|
| 213 |
+
r0(Å)
|
| 214 |
+
Kb(
|
| 215 |
+
kJ
|
| 216 |
+
mol nm2)
|
| 217 |
+
θ0 (deg)
|
| 218 |
+
Kθ ( kJ
|
| 219 |
+
mol)
|
| 220 |
+
φn (deg)
|
| 221 |
+
Kφ ( kJ
|
| 222 |
+
mol)
|
| 223 |
+
n
|
| 224 |
+
3.30
|
| 225 |
+
17000
|
| 226 |
+
130
|
| 227 |
+
85
|
| 228 |
+
180
|
| 229 |
+
1.96
|
| 230 |
+
1
|
| 231 |
+
0
|
| 232 |
+
0.18
|
| 233 |
+
2
|
| 234 |
+
0
|
| 235 |
+
0.33
|
| 236 |
+
3
|
| 237 |
+
0
|
| 238 |
+
0.12
|
| 239 |
+
4
|
| 240 |
+
7
|
| 241 |
+
|
| 242 |
+
PEO2
|
| 243 |
+
PEO2 (CG)The LJ parameters in Eq.1 for CG PEO beads were set to σij = 5 Å and εij = 3.375
|
| 244 |
+
kJ
|
| 245 |
+
mol.
|
| 246 |
+
Each chain in CG PEO modeling has 25 spherical beads connected with the mass mPEO =
|
| 247 |
+
60.05376
|
| 248 |
+
g
|
| 249 |
+
mol.
|
| 250 |
+
System C: Network polymer electrolyte-based supercapacitors
|
| 251 |
+
Nowadays, polymer networks have received much attention due to their characteristics and
|
| 252 |
+
have been used in various applications.29 In network polymer structures, all polymer chains
|
| 253 |
+
are directly or indirectly linked to each other.
|
| 254 |
+
The cross-linking of polymer chains into
|
| 255 |
+
complex networks is a promising strategy to improve the mechanical strength of a GPE and
|
| 256 |
+
provide dimensional stability at high temperatures30 which has been widely investigated.29
|
| 257 |
+
As a model for the polymer network, we consider a cross-link of linear chains as follows.
|
| 258 |
+
First, we highlighted some monomers as cross-links. As the cross-links are closer than the
|
| 259 |
+
distance r0 = 3.30 Å, a new permanent bond is formed between the cross-linkers, acting
|
| 260 |
+
like cross-linked monomers.29 Once equilibrium is reached, the polymer network can be used
|
| 261 |
+
instead of linear polymers in our simulations. Fig. 2a demonstrates the linear polymers we
|
| 262 |
+
consider in our simulation as system B and Fig. 2b displays cross-linked polymers in system
|
| 263 |
+
C.
|
| 264 |
+
Simulation details and electrodes model:
|
| 265 |
+
The simulations were performed using the Langevin thermostat to keep the temperature
|
| 266 |
+
constant.
|
| 267 |
+
Thus, the equation of motion of the system was calculated by the Langevin
|
| 268 |
+
relation:
|
| 269 |
+
m¨ri = −∇iU({ rj(t)}) − γm˙ri + Fi.
|
| 270 |
+
(6)
|
| 271 |
+
The first term describes the deterministic forces between particles (the force acting on atom
|
| 272 |
+
i due to the interaction potentials), and the last two terms implicitly consider the effect of
|
| 273 |
+
the solvent by coupling the system to a Langevin thermostat which maintains a constant
|
| 274 |
+
8
|
| 275 |
+
|
| 276 |
+
(a)
|
| 277 |
+
(b)
|
| 278 |
+
Figure 2: (a) Linear polymers distribution in system B and (b) Cross-linked polymers in
|
| 279 |
+
system C.
|
| 280 |
+
average temperature of the system. The parameter γ is the friction coefficient and Fi is a
|
| 281 |
+
Gaussian distributed random force with31
|
| 282 |
+
⟨Fi(t)⟩ = 0
|
| 283 |
+
⟨Fi(t)Fj(t′)⟩ = 6kBTmγδijδ(t − t′).
|
| 284 |
+
(7)
|
| 285 |
+
Our simulation box included 630 charged particles, where half of which are cations and
|
| 286 |
+
the remains are anions, and 1575 monomers. The density of the bulk region was set to
|
| 287 |
+
1.07
|
| 288 |
+
1
|
| 289 |
+
nm3 and the pore size in three defined systems was equal. To simplify the units, the
|
| 290 |
+
reduced LJ unit was used. The length was scaled with ion size ˜l = σ = 5 Å, and the mass
|
| 291 |
+
unit was ˜m = 144
|
| 292 |
+
g
|
| 293 |
+
mol. The energy unit and the charge unit were ˜ε = 1
|
| 294 |
+
kJ
|
| 295 |
+
mol and ˜q = e.
|
| 296 |
+
By applying ˜t =
|
| 297 |
+
�
|
| 298 |
+
˜mσ2
|
| 299 |
+
˜ε , the time unit was obtained ˜t = 5 ps. In addition, temperature
|
| 300 |
+
9
|
| 301 |
+
|
| 302 |
+
and voltage were scaled as ˜T =
|
| 303 |
+
˜ε
|
| 304 |
+
kB
|
| 305 |
+
= 120.267 ◦K and ˜V = ˜q
|
| 306 |
+
˜ε = 0.01036 V . Temperature
|
| 307 |
+
was kBT = 2.5 ε which corresponded to 300 ◦K in real unit. The friction coefficient in the
|
| 308 |
+
Langevin equation was set to 1
|
| 309 |
+
γ = 1
|
| 310 |
+
˜t and the time step was ∆t = 0.0005 ˜t equal to 6 fs.
|
| 311 |
+
The electrodes were built from carbon atoms with the following parameters: σC = 3.37
|
| 312 |
+
Å and εC = 1
|
| 313 |
+
kJ
|
| 314 |
+
mol.
|
| 315 |
+
Here, using the Poisson to Laplace Transformation (PLT) method,
|
| 316 |
+
which is recently developed in the CAVIAR package,22 the electrodes are surfaces with a
|
| 317 |
+
constant potential. Periodic boundary condition applied in the XY plane and the long-range
|
| 318 |
+
coulombic interaction performed using a 1D Ewald algorithm32 with RC = 15 σ as the cutoff
|
| 319 |
+
distance for electrostatic interaction. The systems were simulated at 17 various potential
|
| 320 |
+
differences between electrodes: 0, 0.25, 0.5, 0.75, 1, 1.25, 1.5, 1.75, 2, 2.25, 2.5, 2.75, 3, 3.25,
|
| 321 |
+
3.5, 3.75, 4 V. Calculations were done after the system reached equilibrium.
|
| 322 |
+
Results and Discussion
|
| 323 |
+
We begin our discussion with a snapshot of three defined systems. Fig.3 illustrates a snap-
|
| 324 |
+
shot from cross-section of the systems configuration and ions separation in the equilibrium
|
| 325 |
+
condition for ∆V = 2 V . In order to find out the charge separation process and the behavior
|
| 326 |
+
of these three systems, it is necessary to conduct numerous calculations and measurements.
|
| 327 |
+
We will discuss this below.
|
| 328 |
+
Charging and Differential Capacitance
|
| 329 |
+
Initially, we discuss the results of the charging process. Fig.4 demonstrates average charge
|
| 330 |
+
density accumulation on the surface of the electrodes for the three systems as a function of the
|
| 331 |
+
applied potential difference between the electrodes. According to the figure, increasing the
|
| 332 |
+
potential difference results in a high concentration of counterions on the electrodes’ surface.
|
| 333 |
+
Therefore average induced charge grows by increasing the applied potential until reaching
|
| 334 |
+
saturation. For system A, the induced charge is greater than in the two other systems. Based
|
| 335 |
+
10
|
| 336 |
+
|
| 337 |
+
15 nm
|
| 338 |
+
4.825 nm
|
| 339 |
+
4.825 nm
|
| 340 |
+
2.5 nm
|
| 341 |
+
8.1 nm
|
| 342 |
+
(a)
|
| 343 |
+
10 nm
|
| 344 |
+
10 nm
|
| 345 |
+
15 nm
|
| 346 |
+
15 nm
|
| 347 |
+
2.5 nm
|
| 348 |
+
(b)
|
| 349 |
+
2.5 nm
|
| 350 |
+
15 nm
|
| 351 |
+
15 nm
|
| 352 |
+
10 nm
|
| 353 |
+
10 nm
|
| 354 |
+
(c)
|
| 355 |
+
Figure 3: The systems configuration at ∆V = 2V after equilibration for (a) System A (b)
|
| 356 |
+
System B and (c) System C.
|
| 357 |
+
on the figure, the saturation voltages for system A is ∆V = 2 V , and for systems B and C is
|
| 358 |
+
∆V = 3.5 V . Since IL-based SCs are saturated at a lower voltage than polymer-based SCs,
|
| 359 |
+
their operating voltage window is also smaller.
|
| 360 |
+
For systems B and C, the induced charges on the electrodes for voltages ∆V < 1.25 V ,
|
| 361 |
+
are almost the same. In voltages, ∆V > 1.25 V , induced charges in system C, are greater
|
| 362 |
+
than system B until both systems reach saturation in ∆V = 3.5 V .
|
| 363 |
+
On the other hand, charge storage in SCs is described by the critical quantities of the
|
| 364 |
+
Differential Capacitance, Cd(V ), and the energy density. The Cd(V ) is the derivative of
|
| 365 |
+
the electrodes surface charge with respect to the applied potential difference between the
|
| 366 |
+
electrodes:33
|
| 367 |
+
Cd(V ) = dq
|
| 368 |
+
dV .
|
| 369 |
+
(8)
|
| 370 |
+
According to the Eq.8, the Cd(V ) is the derivative of the curves in Fig.4. Fig.5, which is
|
| 371 |
+
obtained by the numeric derivation of smooth curves of q(V ), shows the Cd(V ) plots for
|
| 372 |
+
three systems.
|
| 373 |
+
Based on Kornyshev theory for most ILs, Cd(V ) displays a bell-shape, with a maximum at
|
| 374 |
+
11
|
| 375 |
+
|
| 376 |
+
0
|
| 377 |
+
5
|
| 378 |
+
10
|
| 379 |
+
15
|
| 380 |
+
20
|
| 381 |
+
25
|
| 382 |
+
0
|
| 383 |
+
0.5
|
| 384 |
+
1
|
| 385 |
+
1.5
|
| 386 |
+
2
|
| 387 |
+
2.5
|
| 388 |
+
3
|
| 389 |
+
3.5
|
| 390 |
+
4
|
| 391 |
+
Charge Density (µC/cm2)
|
| 392 |
+
Voltage (V)
|
| 393 |
+
System A
|
| 394 |
+
System B
|
| 395 |
+
System C
|
| 396 |
+
Figure 4: Mean induced charge density on the electrodes surface. The points in the figure
|
| 397 |
+
display the simulation data and the solid lines in the plots represent the smoothed data.
|
| 398 |
+
the Potential of Zero Charge (PZC) or a camel-shape with two peaks. In both cases, Cd(V )
|
| 399 |
+
decreases at large potential difference. The reason is, the ions are only allowed to pack up to a
|
| 400 |
+
given maximum density in the double layer. Therefore, by increasing the potential difference,
|
| 401 |
+
the ions concentration near the electrodes’ surface reaches their maximum value and the
|
| 402 |
+
effective diffuse layer thickness actually grows larger, leading to a decrease in Cd(V ).34,34
|
| 403 |
+
Fig.5 is a plot of the Cd(V ) for three systems, which display camel-shaped figures. There
|
| 404 |
+
is limited change in the Cd(V ) curve for system B, indicating the surface charge density
|
| 405 |
+
changes less rapidly in system B with increasing potential. In contrast, there is a peak at
|
| 406 |
+
∆V = 1.5 V in the Cd(V ) plot of system C which points out that more counter-ions can be
|
| 407 |
+
condensed on the electrodes’ surface of system C in comparison with system B. The Cd(V )
|
| 408 |
+
peak for system A is the highest among systems B and C. The result of Korneyshev theory
|
| 409 |
+
is observed in Fig.4 and Fig.5. In systems A, B and C, the saturation voltage is 2, 3 and 3.5
|
| 410 |
+
12
|
| 411 |
+
|
| 412 |
+
0
|
| 413 |
+
2
|
| 414 |
+
4
|
| 415 |
+
6
|
| 416 |
+
8
|
| 417 |
+
10
|
| 418 |
+
12
|
| 419 |
+
14
|
| 420 |
+
16
|
| 421 |
+
0
|
| 422 |
+
0.5
|
| 423 |
+
1
|
| 424 |
+
1.5
|
| 425 |
+
2
|
| 426 |
+
2.5
|
| 427 |
+
3
|
| 428 |
+
3.5
|
| 429 |
+
4
|
| 430 |
+
Differential Capacitance (µF/cm2)
|
| 431 |
+
Voltage (V)
|
| 432 |
+
System A
|
| 433 |
+
System B
|
| 434 |
+
System C
|
| 435 |
+
Figure 5: Differential Capacitance for three systems.
|
| 436 |
+
V . Due to this, in the Cd(V ) plot, the DC drops at voltages above these values.
|
| 437 |
+
As mentioned before, energy density is another useful parameter that shows the efficiency
|
| 438 |
+
of SCs. SC with a higher energy density is more efficient in electrical devices. The stored
|
| 439 |
+
energy density in SCs is obtained:35
|
| 440 |
+
E(V ) =
|
| 441 |
+
� V
|
| 442 |
+
0
|
| 443 |
+
V Cd(V ) dV
|
| 444 |
+
(9)
|
| 445 |
+
Based on the above equation, the plot of energy density for the three systems is calculated
|
| 446 |
+
and plotted in Fig.6. According to this plot, for ∆V < 2 V the energy density of system
|
| 447 |
+
A is greater than systems B and C. For ∆V > 2 V systems B and C have higher energy
|
| 448 |
+
density which indicates that the GPEs-based SC has more efficiency than IL-based SCs in
|
| 449 |
+
higher potential difference.
|
| 450 |
+
13
|
| 451 |
+
|
| 452 |
+
0
|
| 453 |
+
5
|
| 454 |
+
10
|
| 455 |
+
15
|
| 456 |
+
20
|
| 457 |
+
25
|
| 458 |
+
30
|
| 459 |
+
35
|
| 460 |
+
40
|
| 461 |
+
0
|
| 462 |
+
0.5
|
| 463 |
+
1
|
| 464 |
+
1.5
|
| 465 |
+
2
|
| 466 |
+
2.5
|
| 467 |
+
3
|
| 468 |
+
3.5
|
| 469 |
+
4
|
| 470 |
+
Energy Density (µW/cm2)
|
| 471 |
+
Voltage (V)
|
| 472 |
+
System A
|
| 473 |
+
System B
|
| 474 |
+
System C
|
| 475 |
+
Figure 6: The stored energy density in three systems.
|
| 476 |
+
Structural investigation: Ion density profile
|
| 477 |
+
Further insight into the ion structure near the electrodes’ surface is gained in this section.
|
| 478 |
+
Due to the constant density in all three systems, system A has a smaller bulk region between
|
| 479 |
+
its electrodes than systems B and C. It is expected that the ion density profiles will oscillate
|
| 480 |
+
near the charged surface in IL-based SCs,34 as shown in Fig.7a for ∆V = 2 V . Fig.7b and
|
| 481 |
+
Fig.7c depict ion density profiles for systems B and C at ∆V = 2 V after reaching equilibrium.
|
| 482 |
+
Similar to ILs, the ion density profile of these systems exhibits layers and oscillations near
|
| 483 |
+
electrode surfaces. While the conductive electrodes repel co-ions and attract counter-ions,
|
| 484 |
+
co-ions can still be observed inside the pores. The highest peak in Fig.7a can be seen at the
|
| 485 |
+
entrance and end of the pores, which contributes to the high induced charge on the surface
|
| 486 |
+
of the electrodes. Fig.7c, the ion density profile of system C, displays a higher peak at the
|
| 487 |
+
entrance of pores in analogy with the profile of system B. This leads to more induced charge
|
| 488 |
+
14
|
| 489 |
+
|
| 490 |
+
0
|
| 491 |
+
2
|
| 492 |
+
4
|
| 493 |
+
6
|
| 494 |
+
8
|
| 495 |
+
10
|
| 496 |
+
12
|
| 497 |
+
14
|
| 498 |
+
-15
|
| 499 |
+
-10
|
| 500 |
+
-5
|
| 501 |
+
0
|
| 502 |
+
5
|
| 503 |
+
10
|
| 504 |
+
15
|
| 505 |
+
20
|
| 506 |
+
2 V
|
| 507 |
+
0 V
|
| 508 |
+
Ion Density Profile (nm-3)
|
| 509 |
+
X (nm)
|
| 510 |
+
(a)
|
| 511 |
+
0
|
| 512 |
+
2
|
| 513 |
+
4
|
| 514 |
+
6
|
| 515 |
+
8
|
| 516 |
+
10
|
| 517 |
+
12
|
| 518 |
+
14
|
| 519 |
+
-15 -10 -5
|
| 520 |
+
0
|
| 521 |
+
5
|
| 522 |
+
10 15 20 25 30
|
| 523 |
+
2 V
|
| 524 |
+
0 V
|
| 525 |
+
Ion Density Profile (nm-3)
|
| 526 |
+
X (nm)
|
| 527 |
+
(b)
|
| 528 |
+
0
|
| 529 |
+
2
|
| 530 |
+
4
|
| 531 |
+
6
|
| 532 |
+
8
|
| 533 |
+
10
|
| 534 |
+
12
|
| 535 |
+
14
|
| 536 |
+
-15 -10 -5
|
| 537 |
+
0
|
| 538 |
+
5
|
| 539 |
+
10 15 20 25 30
|
| 540 |
+
2 V
|
| 541 |
+
0 V
|
| 542 |
+
Ion Density Profile (nm-3)
|
| 543 |
+
X (nm)
|
| 544 |
+
(c)
|
| 545 |
+
Figure 7: Ion density profile of three systems along x axis for (a) System A (b) System B
|
| 546 |
+
and (c) System C. Green and red graphs display positive and negative ions.
|
| 547 |
+
on the electrodes’ surface and eventually higher energy density.
|
| 548 |
+
The linear polymers can be placed near the electrode surfaces as well as in bulk space in
|
| 549 |
+
system B, in contrast to system C, which places the polymer network only in bulk space. As
|
| 550 |
+
a result, the accessible space for ions near electrode surfaces is reduced. Accordingly, system
|
| 551 |
+
B exhibits a lower ion density at the pore entrance than systems A and C.
|
| 552 |
+
Dynamical investigation: Mean Squared Displacement and
|
| 553 |
+
Diffusion coefficient
|
| 554 |
+
Gels with cross-linked polymers demonstrated higher mobility.5 Since the mobility of ions
|
| 555 |
+
is proportional to the diffusion coefficient (D) we need to calculate the diffusion coefficient.
|
| 556 |
+
The ionic diffusion coefficient is derived from the Mean-Squared Displacement (MSD) curve
|
| 557 |
+
using the 3D diffusion relation:
|
| 558 |
+
MSD ≡< ∆r(t)2 >= 1
|
| 559 |
+
N
|
| 560 |
+
N
|
| 561 |
+
�
|
| 562 |
+
i=1
|
| 563 |
+
< ri(t)2 − ri(0)2 >,
|
| 564 |
+
(10)
|
| 565 |
+
where N is the number of particles. Diffusion coefficient can be calculate using the following
|
| 566 |
+
equation;
|
| 567 |
+
D = lim
|
| 568 |
+
t→∞
|
| 569 |
+
< ∆r(t)2 >
|
| 570 |
+
6t
|
| 571 |
+
.
|
| 572 |
+
(11)
|
| 573 |
+
15
|
| 574 |
+
|
| 575 |
+
According to the above equation, also known as Einstein’s relation,36 the self-diffusion of
|
| 576 |
+
particles is calculated from the slope of the MSD curve over time.
|
| 577 |
+
We calculated MSD for clusters of linear polymers in system B and cross-linked polymers
|
| 578 |
+
in system C. According to Fig.8, MSD for linear polymers and cross-linked polymers display
|
| 579 |
+
superdiffusive motion. On the other hand, by taking the slope of the MSD into account, the
|
| 580 |
+
diffusion coefficient for cross-linked polymers is greater than linear polymers and therefore
|
| 581 |
+
the mobility of cross-linked polymers is higher. This result can also be seen in Fig.9. In this
|
| 582 |
+
figure, two snapshots of both polymers are shown for equal time intervals ∆t = 10 timestep.
|
| 583 |
+
Fig.9a shows lower mobility (for linear polymers) than Fig.9b (for cross-linked polymers).
|
| 584 |
+
0
|
| 585 |
+
0.2
|
| 586 |
+
0.4
|
| 587 |
+
0.6
|
| 588 |
+
0.8
|
| 589 |
+
1
|
| 590 |
+
1.2
|
| 591 |
+
1.4
|
| 592 |
+
1.6
|
| 593 |
+
1.8
|
| 594 |
+
2
|
| 595 |
+
0
|
| 596 |
+
2
|
| 597 |
+
4
|
| 598 |
+
6
|
| 599 |
+
8
|
| 600 |
+
10
|
| 601 |
+
12
|
| 602 |
+
~ t1.91
|
| 603 |
+
~ t1.99
|
| 604 |
+
Mean Squared Displacement (× 106 nm2)
|
| 605 |
+
Time (ns)
|
| 606 |
+
Linear polymers in system B
|
| 607 |
+
Network polymer in system C
|
| 608 |
+
1×10-5
|
| 609 |
+
1×10-4
|
| 610 |
+
1×10-3
|
| 611 |
+
1×10-2
|
| 612 |
+
1×10-1
|
| 613 |
+
1×100
|
| 614 |
+
1×101
|
| 615 |
+
1×10-1
|
| 616 |
+
1×100
|
| 617 |
+
1×101
|
| 618 |
+
Figure 8: Mean Squared Displacement of polymers in systems B and C in absence of electric
|
| 619 |
+
field. Inner is the same result but in logarithmic scale, indicating on power-law behavior of
|
| 620 |
+
MSD.
|
| 621 |
+
In addition, we obtained MSD for cations and anions for all systems. Due to volume
|
| 622 |
+
effects and the high mobility of cross-linked polymers, these polymers provide a limited path
|
| 623 |
+
for charged particles in system C in comparison with linear polymers in system B. Therefore
|
| 624 |
+
16
|
| 625 |
+
|
| 626 |
+
(a)
|
| 627 |
+
(b)
|
| 628 |
+
Figure 9: Two different snapshots of polymers for (a) linear polymers in system B and (b)
|
| 629 |
+
cross-linked polymers in system C.
|
| 630 |
+
as shown in Fig.10, the charged particles’ diffusion in system C is lower than in systems A
|
| 631 |
+
and B. Since a lower diffusion coefficient is associated with a larger viscosity, the viscosity
|
| 632 |
+
of system C is greater than systems A and B. Consequently, increasing the viscosity of the
|
| 633 |
+
electrolyte improves its mechanical stability. Accordingly, system C has higher mechanical
|
| 634 |
+
stability than systems A and B.
|
| 635 |
+
Furthermore, it is important to note that cations and anions differ slightly in their results
|
| 636 |
+
due to their mass differences. Compared to a cation, an anion has a lower weight, so its
|
| 637 |
+
MSD plot shows a higher value.
|
| 638 |
+
17
|
| 639 |
+
|
| 640 |
+
0
|
| 641 |
+
1
|
| 642 |
+
2
|
| 643 |
+
3
|
| 644 |
+
4
|
| 645 |
+
5
|
| 646 |
+
6
|
| 647 |
+
7
|
| 648 |
+
8
|
| 649 |
+
9
|
| 650 |
+
0
|
| 651 |
+
2
|
| 652 |
+
4
|
| 653 |
+
6
|
| 654 |
+
8
|
| 655 |
+
10
|
| 656 |
+
12
|
| 657 |
+
D ~ 0.21538 × 10-4 (m2/s)
|
| 658 |
+
D ~ 0.1375 × 10-4 (m2/s)
|
| 659 |
+
D ~ 0.07313 × 10-4 (m2/s)
|
| 660 |
+
Mean Squared Displacement (× 105 nm2)
|
| 661 |
+
Time (ns)
|
| 662 |
+
anion in system A
|
| 663 |
+
cation in system A
|
| 664 |
+
anion in system B
|
| 665 |
+
cation in system B
|
| 666 |
+
anion in system C
|
| 667 |
+
cation in system C
|
| 668 |
+
1×10-4
|
| 669 |
+
1×10-3
|
| 670 |
+
1×10-2
|
| 671 |
+
1×10-1
|
| 672 |
+
1×100
|
| 673 |
+
1×101
|
| 674 |
+
1×10-1
|
| 675 |
+
1×100
|
| 676 |
+
1×101
|
| 677 |
+
Figure 10: Mean Squared Displacement of ions in all three systems at ∆V = 2 V . Inner plot
|
| 678 |
+
is the same as outer but in logarithmic scale.
|
| 679 |
+
Conclusion
|
| 680 |
+
In summary, simulations demonstrate a difference between the performance of two types
|
| 681 |
+
of electrolytes, i.e. liquid and solid electrolytes in supercapacitors. Solid electrolytes are
|
| 682 |
+
used as an alternative to reduce the problems associated with liquid electrolytes. Therefore,
|
| 683 |
+
simulation and comparison of these two categories can give us a clear insight into improving
|
| 684 |
+
the efficiency of supercapacitors.
|
| 685 |
+
Liquid electrolyte-based supercapacitors have a smaller operating voltage window there-
|
| 686 |
+
fore, the amount of energy stored is less. Polymer electrolytes can be considered as a cluster
|
| 687 |
+
of linear polymers or as cross-linked polymers in which linear polymers are connected and
|
| 688 |
+
form a network. In linear polymers, since polymers can be present near the walls of the elec-
|
| 689 |
+
trodes as well as inside the pores, the available space for ions in the vicinity of the electrodes
|
| 690 |
+
is reduced. In contrast, in a polymer network, the movement of polymers is collective, and
|
| 691 |
+
18
|
| 692 |
+
|
| 693 |
+
therefore polymers can only be present in bulk space. Therefore, the accessible space for
|
| 694 |
+
ions near the surfaces of the two electrodes and inside the pores increases. So the amount
|
| 695 |
+
of charge stored in the electrodes and the supercapacitor efficiency increases.
|
| 696 |
+
19
|
| 697 |
+
|
| 698 |
+
References
|
| 699 |
+
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|
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oid sha256:5250535ed4e961edc5e1ed88533f4ea58a72d495e0b480c7c6082f602e84ffd2
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| 3 |
+
size 81117
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F9FJT4oBgHgl3EQfDixl/content/tmp_files/2301.11434v1.pdf.txt
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|
| 1 |
+
|
| 2 |
+
|
| 3 |
+
|
| 4 |
+
The Field Structure of Free Photons
|
| 5 |
+
|
| 6 |
+
Anthony Rizzi
|
| 7 |
+
Institute for Advanced Physics, arizzi@iapweb.org
|
| 8 |
+
|
| 9 |
+
Abstract: Using a quantum field theoretic description of the photon it is shown that, as
|
| 10 |
+
intuitively expected but not before theoretically proven, the vector potential of a photon
|
| 11 |
+
has a likely amplitude associated with a discrete frequency and therefore energy, and
|
| 12 |
+
momentum. In particular, by finding the wave-functional for the vector potential, it is
|
| 13 |
+
shown that the likely absolute amplitude spectrum has delta function at a given
|
| 14 |
+
frequency. This analysis is extended to n-photon systems. It shows that such systems
|
| 15 |
+
have a vector potential distribution whose most likely element has a strong sinusoidal
|
| 16 |
+
component which has an amplitude corresponding to n-fold more energy than a single
|
| 17 |
+
photon system. An analogous result for photons of different energy is also derived.
|
| 18 |
+
Through the use of Parseval’s theorem for stochastic systems, the calculations and
|
| 19 |
+
associated analyses introduces a simple tool for exploring the nature of QFT Schrödinger
|
| 20 |
+
wave-functional generally.
|
| 21 |
+
|
| 22 |
+
Introduction
|
| 23 |
+
|
| 24 |
+
Photons are discussed everywhere from middle school, even grade school, to
|
| 25 |
+
graduate textbooks and beyond and are a core part of modern physics, but proving and
|
| 26 |
+
show their field structure, the focus of this article, has not been a part of these
|
| 27 |
+
discussions. Rules of thumb and intuitions from ordinary quantum mechanics and
|
| 28 |
+
quantum optics abound. But, as we know, these do not substitute for rigorous analysis
|
| 29 |
+
from first principles from what we know theoretically. And, what we know theoretically
|
| 30 |
+
about photons is contained in quantum field theory. Ordinary quantum mechanics and
|
| 31 |
+
quantum optics studies can only handle photons to the extent information is imported
|
| 32 |
+
from QFT. This paper for the first time directly applies the relevant QFT to obtain the full
|
| 33 |
+
probabilistic structure of the photon’s vector potential (which is what specifies what it is)
|
| 34 |
+
towards proving its key property, its discrete energy nature. In the process, a new
|
| 35 |
+
technique for probing such structures is introduced. Though QFT is a mature part of
|
| 36 |
+
physics, no one has yet shown the nature of a photon using QFT in the primal way done
|
| 37 |
+
here. Seeing this structure and how it connects to our previous intuitions is an essential
|
| 38 |
+
insight into the physics of photons, which, in turn, are at the center of modern physics.
|
| 39 |
+
|
| 40 |
+
Much previous work has been done in trying to probe the nature of the photon,1
|
| 41 |
+
beginning with the early investigations trying to “split” the photon.2 Free photons are
|
| 42 |
+
often discussed as if they were localized particles, but they are not. Of course, photons by
|
| 43 |
+
definition cause localized detections, but, as this article, proves their most likely field
|
| 44 |
+
structure is, in the idealized limit, an infinite length sine wave of undetermined phase.
|
| 45 |
+
This agrees with the natural understanding of a photon as a packet of definite energy (and
|
| 46 |
+
thus definite frequency), but makes it clear that even though when it interacts, it interacts
|
| 47 |
+
|
| 48 |
+
1 E.G., see special issue on nature of photon: Optics and Photonics News (vol. 14, October 2003).
|
| 49 |
+
2 E. O. Lawrence, J. W. Beams, On the Nature of Light, PNAS 13 No. 4, 207-212 (1927), G. P. Thomson,
|
| 50 |
+
Test of a Theory of Radiation, Proceedings of the Royal Society of London. Series A, Containing Papers of
|
| 51 |
+
a Mathematical and Physical Character 104 No. 724, 115-120 (1923).
|
| 52 |
+
|
| 53 |
+
2
|
| 54 |
+
|
| 55 |
+
locally (e.g., with an atom), when it is free, before it begins to interact (with an atom for
|
| 56 |
+
example), its wave structure is spread out, not a localized wave packet.3 Giving (via
|
| 57 |
+
proofs) the structure of the photon offers us insights into simplest QFT structure, the free
|
| 58 |
+
photon, and thus can be a first glimpse of a deeper view of the nature of QFT itself as
|
| 59 |
+
well as a formalisms that has seldom been used, the Schrödinger wavefunctional and a
|
| 60 |
+
statistical formalism that has not been yet applied in QFT.
|
| 61 |
+
|
| 62 |
+
Up to this point, photon structure has been, indeed, taken for granted as issues
|
| 63 |
+
related to a wide range of important problems were discussed. These extend from trying
|
| 64 |
+
to find analogs of ordinary of wavefunctions for the spatially limited photon as well as its
|
| 65 |
+
associated probability for locating a photon, separately developing probability
|
| 66 |
+
distributions for detecting a photon based on an electric field operator, finding energy
|
| 67 |
+
distribution functions of such spatially limited photons to studying correlation functions
|
| 68 |
+
and coherent states created as superposition of Fock states and photon interference
|
| 69 |
+
phenomena as well as light squeezing.4 These problems are addressed using various
|
| 70 |
+
approaches, but seldom, if ever, use the QFT formalism of the Schrödinger
|
| 71 |
+
wavefunctional. The most natural approach to the photon field structure is this
|
| 72 |
+
Schrödinger formalism in combination with the commonly used Fock formalism. Now,
|
| 73 |
+
each formalism facilitates a different insight into the physics of a given system. Feynman
|
| 74 |
+
once said that every theorist should know many ways to solve the same problem.5 The
|
| 75 |
+
Schrödinger wavefunctional formalism has been somewhat neglected in this regard. In
|
| 76 |
+
ordinary quantum mechanics, the Schrödinger equation is usually preferentially used in
|
| 77 |
+
both teaching and applications. In ordinary QM, the S-matrix type approach and other
|
| 78 |
+
approaches (e.g. Green functions and path integrals) have their place and are used, but do
|
| 79 |
+
not eclipse the Schrödinger equation. By contrast in QFT teaching and applications, the
|
| 80 |
+
analogous Schrödinger wave functional equation is left out almost completely (along
|
| 81 |
+
with all the intuitive advantages it affords). Few resources use or even mention it.6,7
|
| 82 |
+
Because of this, we first review those little known results of the analysis for our case and
|
| 83 |
+
then move to understand what they imply. Deriving those results is helpful in clearly
|
| 84 |
+
|
| 85 |
+
3 This is sometimes alluded to but usually vaguely but, in the literature as far as I could find, always
|
| 86 |
+
without proof.
|
| 87 |
+
4 See for example R. Loudon, The Quantum Theory of Light Third Edition (Oxford University Press, New
|
| 88 |
+
York, 2000) and L. Mandel, E. Wolf, Optical Coherence and Quantum Optics (Cambridge, NY, 1995)
|
| 89 |
+
5 “Every theoretical physicist who is any good knows six or seven different theoretical representations for
|
| 90 |
+
exactly the same physics. He knows that they are all equivalent, and that nobody is ever going to be able
|
| 91 |
+
to decide which one is right at that level, but he keeps them in his head, hoping that they will give him
|
| 92 |
+
different ideas for guessing.” Feynman, MIT Press Character of Physical Law (1985), 168.
|
| 93 |
+
6 Quantum field theory textbooks that I am aware of do not mention it. For example, the following first rate
|
| 94 |
+
texts do not discuss Schrödinger wavefuntionals: F. Mandl and G. Shaw, Quantum Field Theory (2nd ed,
|
| 95 |
+
Wiley, West Sussex 2010), P. Ramond, Field Theory: A Modern Primer (2nd ed, Westview Press, Boulder
|
| 96 |
+
2001), C. Itzykson and J. Zuber, Quantum Field Theory (McGraw-Hill, USA 1980), M. Peskin and D.
|
| 97 |
+
Schroeder, Quantum Field Theory (Perseus Books, MA 1995), M. Kaku, Quantum Field Theory: A Modern
|
| 98 |
+
Introduction (Oxford University Press, NY 1993), A. Zee, Quantum Field Theory in a Nutshell (Princeton
|
| 99 |
+
Univ. Press, NJ 2003). W. Greiner and J. Reinhardt, Field Quantization (Springer-Verlag, Berlin, 1996). S.
|
| 100 |
+
Weinberg, The Quantum Theory of Fields, Volume I and II (Cambridge University Press, NY 1995, 1996).
|
| 101 |
+
7 K. Symanzik, Schrodinger Representation and Casimir Effect in Renormalizable Quantum Field Theory,
|
| 102 |
+
Nucl. Phys. B 190, 1-44 (1981) showed the Schrödinger representation was renormalizable. These paper
|
| 103 |
+
discuss it: B. Hatfield, Quantum Field Theory of Point Particles and Strings (Perseus, Cambrdige MA,
|
| 104 |
+
1992), R. Jackiw, Analysis on Infinite-Dimensional Manifolds Schrödinger Representation for Quantized
|
| 105 |
+
Fields in Field Theory and Particle Physics, O. Eboli, et al. eds. (World Scientific, Brazil, 1989) 78-143p.
|
| 106 |
+
|
| 107 |
+
3
|
| 108 |
+
|
| 109 |
+
understanding the approach’s fundamental nature and hopefully in spawning its further
|
| 110 |
+
use.
|
| 111 |
+
|
| 112 |
+
In section 1, first the basic formalism is introduced in the process of setting up the
|
| 113 |
+
calculation for the field structure of the single photon wave functional. Next, Parseval’s
|
| 114 |
+
theorem is introduced to analyze that structure statistically, as it must be since the
|
| 115 |
+
quantum mechanical vector potential is fundamentally stochastic. This statistical
|
| 116 |
+
formalism is commonly used, for example, in electrical engineering where one looks,
|
| 117 |
+
amidst noise, for the spectral content of a signal.8 This is fundamentally is needed here.
|
| 118 |
+
The calculation shows that the amplitude of A for the single photon of momentum p is as
|
| 119 |
+
intuitively expected sinusoidal of the frequency
|
| 120 |
+
/ h
|
| 121 |
+
ν = p
|
| 122 |
+
.
|
| 123 |
+
|
| 124 |
+
In section 2, the formalism is generalized to the case of n identical free photons;
|
| 125 |
+
the full explicit form of the wavefunctional is given up to 4 photons and then the core
|
| 126 |
+
form of the n-photon wavefunctional is given. In section 3, the multi-photon case with
|
| 127 |
+
different momenta is resolved by giving the explicit results for the two photon different-
|
| 128 |
+
momenta case. In each of these last two sections, the results prove that 1-photon
|
| 129 |
+
sinusoidal structure is found, as intuitively expected, also in the general n-photon
|
| 130 |
+
systems.
|
| 131 |
+
|
| 132 |
+
We take metric,
|
| 133 |
+
μν
|
| 134 |
+
η
|
| 135 |
+
, to have signature (
|
| 136 |
+
)
|
| 137 |
+
, , ,
|
| 138 |
+
+ − − − and components {
|
| 139 |
+
}
|
| 140 |
+
0,1,2,3 and
|
| 141 |
+
1
|
| 142 |
+
=
|
| 143 |
+
�
|
| 144 |
+
, and, ultimately,
|
| 145 |
+
1
|
| 146 |
+
c = .
|
| 147 |
+
Single Photon Wave-functional
|
| 148 |
+
|
| 149 |
+
Assuming one is operating in the Lorenz gauge, where the classical equations of
|
| 150 |
+
motion are separable, we get the equations for the vector potential components in the
|
| 151 |
+
presence of a current source:
|
| 152 |
+
(1)
|
| 153 |
+
|
| 154 |
+
|
| 155 |
+
|
| 156 |
+
2
|
| 157 |
+
2
|
| 158 |
+
2
|
| 159 |
+
2
|
| 160 |
+
1
|
| 161 |
+
4
|
| 162 |
+
A
|
| 163 |
+
A
|
| 164 |
+
J
|
| 165 |
+
c
|
| 166 |
+
t
|
| 167 |
+
c
|
| 168 |
+
μ
|
| 169 |
+
μ
|
| 170 |
+
μ
|
| 171 |
+
π
|
| 172 |
+
∂
|
| 173 |
+
− ∇
|
| 174 |
+
=
|
| 175 |
+
∂
|
| 176 |
+
|
| 177 |
+
|
| 178 |
+
|
| 179 |
+
We are not here interested in the production of the fields, so we consider only the
|
| 180 |
+
source-less case, which can arise from considering only regions sufficiently far from the
|
| 181 |
+
sources or, for conceptual simplicity, we can simply posit a given field of radiation as an
|
| 182 |
+
initial condition. Furthermore, since our interest is in radiation, for which the scalar
|
| 183 |
+
potential is not needed, we simply ignore it.9 This leaves taking
|
| 184 |
+
1
|
| 185 |
+
c = and using the
|
| 186 |
+
Einstein summation convention:
|
| 187 |
+
(2)
|
| 188 |
+
|
| 189 |
+
|
| 190 |
+
( )
|
| 191 |
+
( )
|
| 192 |
+
2
|
| 193 |
+
0,
|
| 194 |
+
j
|
| 195 |
+
i
|
| 196 |
+
i
|
| 197 |
+
A
|
| 198 |
+
x
|
| 199 |
+
A
|
| 200 |
+
x
|
| 201 |
+
− ∂
|
| 202 |
+
=
|
| 203 |
+
��
|
| 204 |
+
where x is the 4-vector coordinate.
|
| 205 |
+
|
| 206 |
+
|
| 207 |
+
(this EOM is associated with
|
| 208 |
+
2
|
| 209 |
+
2
|
| 210 |
+
1
|
| 211 |
+
1
|
| 212 |
+
2
|
| 213 |
+
2
|
| 214 |
+
i
|
| 215 |
+
i
|
| 216 |
+
i
|
| 217 |
+
A
|
| 218 |
+
A
|
| 219 |
+
m A
|
| 220 |
+
ν
|
| 221 |
+
μ
|
| 222 |
+
=
|
| 223 |
+
∂
|
| 224 |
+
∂
|
| 225 |
+
−
|
| 226 |
+
L
|
| 227 |
+
, the spatial Proca
|
| 228 |
+
|
| 229 |
+
|
| 230 |
+
Lagrangian, with
|
| 231 |
+
0
|
| 232 |
+
m =
|
| 233 |
+
)
|
| 234 |
+
|
| 235 |
+
8 R. M. Howard, Principles of Random Signal Analysis and Low Noise Design: The Power Spectral Density
|
| 236 |
+
and Its Applications (John Wiley & Sons, 2002).
|
| 237 |
+
9 In this way, we sidestep problems with quantizing the full special relativistic field ( Aμ ) in the Lorentz
|
| 238 |
+
gauge. A more formal way to ignore the scalar potential is assume an arbitrarily small mass (rather than
|
| 239 |
+
zero mass) in the Proca Lagrangian and then use the Lorenz gauge condition to eliminate the scalar
|
| 240 |
+
potential (since in the massive case there are three independent degrees of freedom, rather than the two of
|
| 241 |
+
the massless field).
|
| 242 |
+
|
| 243 |
+
4
|
| 244 |
+
|
| 245 |
+
|
| 246 |
+
Moving to second quantization operators, recalling the classical canonical
|
| 247 |
+
momentum
|
| 248 |
+
( )
|
| 249 |
+
( ) /
|
| 250 |
+
i
|
| 251 |
+
i
|
| 252 |
+
x
|
| 253 |
+
A x
|
| 254 |
+
t
|
| 255 |
+
π
|
| 256 |
+
≡ ∂
|
| 257 |
+
∂ , this equation implies the following Hamiltonian operator
|
| 258 |
+
in Heisenberg picture.
|
| 259 |
+
(3)
|
| 260 |
+
|
| 261 |
+
|
| 262 |
+
(
|
| 263 |
+
)
|
| 264 |
+
3
|
| 265 |
+
2
|
| 266 |
+
1
|
| 267 |
+
ˆ
|
| 268 |
+
ˆ
|
| 269 |
+
ˆ
|
| 270 |
+
ˆ
|
| 271 |
+
( , )
|
| 272 |
+
( , )·
|
| 273 |
+
( , ) ,
|
| 274 |
+
2
|
| 275 |
+
i
|
| 276 |
+
i
|
| 277 |
+
i
|
| 278 |
+
H
|
| 279 |
+
t
|
| 280 |
+
A
|
| 281 |
+
t
|
| 282 |
+
A
|
| 283 |
+
t
|
| 284 |
+
d
|
| 285 |
+
π
|
| 286 |
+
=
|
| 287 |
+
+ ∇
|
| 288 |
+
∇
|
| 289 |
+
∫
|
| 290 |
+
x
|
| 291 |
+
x
|
| 292 |
+
x
|
| 293 |
+
x
|
| 294 |
+
|
| 295 |
+
|
| 296 |
+
where we impose (equal time) canonical quantization:9
|
| 297 |
+
|
| 298 |
+
|
| 299 |
+
|
| 300 |
+
ˆ
|
| 301 |
+
ˆ
|
| 302 |
+
[
|
| 303 |
+
( , ),
|
| 304 |
+
( , )]
|
| 305 |
+
(
|
| 306 |
+
)
|
| 307 |
+
i
|
| 308 |
+
j
|
| 309 |
+
ij
|
| 310 |
+
A
|
| 311 |
+
t
|
| 312 |
+
t
|
| 313 |
+
i
|
| 314 |
+
π
|
| 315 |
+
δ δ
|
| 316 |
+
=
|
| 317 |
+
−
|
| 318 |
+
′
|
| 319 |
+
x
|
| 320 |
+
x
|
| 321 |
+
x
|
| 322 |
+
x
|
| 323 |
+
.
|
| 324 |
+
Thus, the Schrödinger equation for the wave functional Ψ is: 10
|
| 325 |
+
(4)
|
| 326 |
+
|
| 327 |
+
(
|
| 328 |
+
)
|
| 329 |
+
(
|
| 330 |
+
)
|
| 331 |
+
(
|
| 332 |
+
)
|
| 333 |
+
2
|
| 334 |
+
2
|
| 335 |
+
3
|
| 336 |
+
2
|
| 337 |
+
1
|
| 338 |
+
2
|
| 339 |
+
ˆ
|
| 340 |
+
i
|
| 341 |
+
i
|
| 342 |
+
i
|
| 343 |
+
iA
|
| 344 |
+
A
|
| 345 |
+
i
|
| 346 |
+
d x
|
| 347 |
+
A
|
| 348 |
+
t
|
| 349 |
+
A
|
| 350 |
+
δ
|
| 351 |
+
δ
|
| 352 |
+
∂Ψ
|
| 353 |
+
⎛
|
| 354 |
+
⎞
|
| 355 |
+
=
|
| 356 |
+
−
|
| 357 |
+
+ ∇
|
| 358 |
+
Ψ
|
| 359 |
+
⎜
|
| 360 |
+
⎟
|
| 361 |
+
∂
|
| 362 |
+
⎝
|
| 363 |
+
⎠
|
| 364 |
+
∫
|
| 365 |
+
,
|
| 366 |
+
Here we used:
|
| 367 |
+
(5)
|
| 368 |
+
|
| 369 |
+
|
| 370 |
+
ˆ
|
| 371 |
+
ˆ
|
| 372 |
+
i
|
| 373 |
+
i
|
| 374 |
+
i
|
| 375 |
+
i
|
| 376 |
+
i
|
| 377 |
+
i
|
| 378 |
+
A
|
| 379 |
+
A
|
| 380 |
+
A
|
| 381 |
+
δ
|
| 382 |
+
δ
|
| 383 |
+
π
|
| 384 |
+
δ
|
| 385 |
+
δ
|
| 386 |
+
⎛
|
| 387 |
+
⎞
|
| 388 |
+
=
|
| 389 |
+
→ −
|
| 390 |
+
=
|
| 391 |
+
⎜
|
| 392 |
+
⎟
|
| 393 |
+
⎝
|
| 394 |
+
⎠
|
| 395 |
+
�
|
| 396 |
+
|
| 397 |
+
The free solution (in the Heisenberg picture) for the vector potential operator is, taking
|
| 398 |
+
motion along z-axis, and assuming only one polarization (thereby also limiting A
|
| 399 |
+
eigenstates, A , to one polarization at a time 11):12,13
|
| 400 |
+
(6)
|
| 401 |
+
( ) (
|
| 402 |
+
)
|
| 403 |
+
(
|
| 404 |
+
)
|
| 405 |
+
( ) ( )
|
| 406 |
+
( ) ( )
|
| 407 |
+
(
|
| 408 |
+
)
|
| 409 |
+
3
|
| 410 |
+
†
|
| 411 |
+
3/2
|
| 412 |
+
1
|
| 413 |
+
ˆ
|
| 414 |
+
ˆ
|
| 415 |
+
ˆ
|
| 416 |
+
,
|
| 417 |
+
2
|
| 418 |
+
2
|
| 419 |
+
i
|
| 420 |
+
i
|
| 421 |
+
i
|
| 422 |
+
i
|
| 423 |
+
d p
|
| 424 |
+
t
|
| 425 |
+
a
|
| 426 |
+
t e
|
| 427 |
+
a
|
| 428 |
+
t
|
| 429 |
+
A
|
| 430 |
+
e
|
| 431 |
+
E
|
| 432 |
+
λ
|
| 433 |
+
λ
|
| 434 |
+
λ
|
| 435 |
+
λ
|
| 436 |
+
δ
|
| 437 |
+
π
|
| 438 |
+
⋅
|
| 439 |
+
−
|
| 440 |
+
⋅
|
| 441 |
+
=
|
| 442 |
+
+
|
| 443 |
+
∫
|
| 444 |
+
p x
|
| 445 |
+
p x
|
| 446 |
+
p
|
| 447 |
+
p
|
| 448 |
+
p
|
| 449 |
+
x
|
| 450 |
+
|
| 451 |
+
|
| 452 |
+
|
| 453 |
+
|
| 454 |
+
|
| 455 |
+
|
| 456 |
+
where:
|
| 457 |
+
( ) ( )
|
| 458 |
+
( )
|
| 459 |
+
ˆ
|
| 460 |
+
ˆ
|
| 461 |
+
iEt
|
| 462 |
+
a
|
| 463 |
+
t
|
| 464 |
+
a
|
| 465 |
+
e
|
| 466 |
+
λ
|
| 467 |
+
λ
|
| 468 |
+
−
|
| 469 |
+
=
|
| 470 |
+
p
|
| 471 |
+
p
|
| 472 |
+
,
|
| 473 |
+
p
|
| 474 |
+
E = p ,
|
| 475 |
+
(
|
| 476 |
+
)
|
| 477 |
+
0,0, p
|
| 478 |
+
=
|
| 479 |
+
p
|
| 480 |
+
|
| 481 |
+
|
| 482 |
+
|
| 483 |
+
|
| 484 |
+
|
| 485 |
+
|
| 486 |
+
|
| 487 |
+
{
|
| 488 |
+
}
|
| 489 |
+
1,2
|
| 490 |
+
λ ∈
|
| 491 |
+
, (two independent polarizations)
|
| 492 |
+
From here on, we will usually drop the formal t dependence of the creation and
|
| 493 |
+
annihilation operators, so that by also dropping explicit polarization notation (by taking
|
| 494 |
+
i
|
| 495 |
+
λ → ), we can write simply ˆi
|
| 496 |
+
p
|
| 497 |
+
a . So,
|
| 498 |
+
|
| 499 |
+
|
| 500 |
+
with
|
| 501 |
+
†
|
| 502 |
+
†
|
| 503 |
+
ˆ
|
| 504 |
+
ˆ
|
| 505 |
+
ˆ
|
| 506 |
+
ˆ
|
| 507 |
+
,
|
| 508 |
+
,
|
| 509 |
+
0
|
| 510 |
+
a
|
| 511 |
+
a
|
| 512 |
+
a
|
| 513 |
+
a
|
| 514 |
+
′
|
| 515 |
+
′
|
| 516 |
+
⎡
|
| 517 |
+
⎤
|
| 518 |
+
⎡
|
| 519 |
+
⎤ =
|
| 520 |
+
=
|
| 521 |
+
⎣
|
| 522 |
+
⎦
|
| 523 |
+
⎣
|
| 524 |
+
⎦
|
| 525 |
+
p
|
| 526 |
+
p
|
| 527 |
+
p
|
| 528 |
+
p
|
| 529 |
+
,
|
| 530 |
+
(
|
| 531 |
+
)
|
| 532 |
+
†
|
| 533 |
+
ˆ
|
| 534 |
+
ˆ
|
| 535 |
+
,
|
| 536 |
+
a
|
| 537 |
+
a
|
| 538 |
+
δ
|
| 539 |
+
′
|
| 540 |
+
′
|
| 541 |
+
⎡
|
| 542 |
+
⎤ =
|
| 543 |
+
−
|
| 544 |
+
⎣
|
| 545 |
+
⎦
|
| 546 |
+
p
|
| 547 |
+
p
|
| 548 |
+
p
|
| 549 |
+
p
|
| 550 |
+
,
|
| 551 |
+
|
| 552 |
+
|
| 553 |
+
|
| 554 |
+
|
| 555 |
+
|
| 556 |
+
†
|
| 557 |
+
3
|
| 558 |
+
1
|
| 559 |
+
ˆ
|
| 560 |
+
ˆ ˆ
|
| 561 |
+
2
|
| 562 |
+
H
|
| 563 |
+
E
|
| 564 |
+
a a
|
| 565 |
+
d p
|
| 566 |
+
⎛
|
| 567 |
+
⎞
|
| 568 |
+
=
|
| 569 |
+
+
|
| 570 |
+
⎜
|
| 571 |
+
⎟
|
| 572 |
+
⎝
|
| 573 |
+
⎠
|
| 574 |
+
∫
|
| 575 |
+
p
|
| 576 |
+
p
|
| 577 |
+
p
|
| 578 |
+
.
|
| 579 |
+
Adding (6) to its time derivative and taking the Fourier transform gives, dropping the
|
| 580 |
+
polarization index from A:
|
| 581 |
+
(7)
|
| 582 |
+
|
| 583 |
+
(
|
| 584 |
+
)
|
| 585 |
+
(
|
| 586 |
+
)
|
| 587 |
+
(
|
| 588 |
+
)
|
| 589 |
+
(
|
| 590 |
+
)
|
| 591 |
+
3
|
| 592 |
+
3/2
|
| 593 |
+
1
|
| 594 |
+
1
|
| 595 |
+
ˆ
|
| 596 |
+
,
|
| 597 |
+
ˆ
|
| 598 |
+
ˆ
|
| 599 |
+
,
|
| 600 |
+
2
|
| 601 |
+
2
|
| 602 |
+
i
|
| 603 |
+
i
|
| 604 |
+
i
|
| 605 |
+
i
|
| 606 |
+
a
|
| 607 |
+
E
|
| 608 |
+
t
|
| 609 |
+
A
|
| 610 |
+
A
|
| 611 |
+
i
|
| 612 |
+
t
|
| 613 |
+
e
|
| 614 |
+
d x
|
| 615 |
+
E
|
| 616 |
+
π
|
| 617 |
+
−
|
| 618 |
+
⋅
|
| 619 |
+
=
|
| 620 |
+
+
|
| 621 |
+
∫
|
| 622 |
+
�
|
| 623 |
+
p x
|
| 624 |
+
p
|
| 625 |
+
p
|
| 626 |
+
p
|
| 627 |
+
x
|
| 628 |
+
x
|
| 629 |
+
|
| 630 |
+
|
| 631 |
+
|
| 632 |
+
10 The equation is the field theory analog, for a given spectral mode of A at each point in space, of the
|
| 633 |
+
ordinary quantum mechanical oscillator.
|
| 634 |
+
11 Note this still preserves the commutation relations (since it becomes analogical to the scalar field case).
|
| 635 |
+
12 The equation of motion for the vector potential operator can be shown, via the quantum generalization of
|
| 636 |
+
Hamilton’s equations, to be the analog of the classical vector potential field’s equation of motion.
|
| 637 |
+
13 Note the measure in the integrand is not manifestly relativistic invariant, the manifestly Lorentz
|
| 638 |
+
invariant:
|
| 639 |
+
(
|
| 640 |
+
)
|
| 641 |
+
4
|
| 642 |
+
2
|
| 643 |
+
2
|
| 644 |
+
0
|
| 645 |
+
(
|
| 646 |
+
)
|
| 647 |
+
d
|
| 648 |
+
m
|
| 649 |
+
u p
|
| 650 |
+
p
|
| 651 |
+
p
|
| 652 |
+
δ
|
| 653 |
+
−
|
| 654 |
+
reduces, after integrating over p0 and with appropriate normalization, to
|
| 655 |
+
the 3D measure given in the text body. Note that a factor of 1 /
|
| 656 |
+
2E has been absorbed into the definition
|
| 657 |
+
of the creation operators to avoid a factor of 2E in the creation operator commutation relations.
|
| 658 |
+
|
| 659 |
+
5
|
| 660 |
+
|
| 661 |
+
|
| 662 |
+
Note: x is the spatial coordinate.
|
| 663 |
+
|
| 664 |
+
|
| 665 |
+
Now, noting that the QFT creation operators are analogous to the creation and
|
| 666 |
+
annihilation operators of the quantum mechanical harmonic oscillator (QMHO)
|
| 667 |
+
( ˆ
|
| 668 |
+
ˆ
|
| 669 |
+
ˆ
|
| 670 |
+
~
|
| 671 |
+
a
|
| 672 |
+
x
|
| 673 |
+
p
|
| 674 |
+
+
|
| 675 |
+
), we can apply the well known formal method of calculating the QMHO
|
| 676 |
+
energy eigenfunctions to calculate the wave-functionals of the n-photon (free) A-field.
|
| 677 |
+
We start with the one photon case.
|
| 678 |
+
|
| 679 |
+
In particular, using (5) in (7), we define the relevant wave functional as the
|
| 680 |
+
probability amplitude for finding a field which is prepared in the state called a (ideal)
|
| 681 |
+
“single photon of momentum p” (and described by the ket
|
| 682 |
+
† 0
|
| 683 |
+
a
|
| 684 |
+
=
|
| 685 |
+
p
|
| 686 |
+
p
|
| 687 |
+
) in the state
|
| 688 |
+
iA
|
| 689 |
+
, which is the eigenstate of
|
| 690 |
+
( )
|
| 691 |
+
ˆ iA
|
| 692 |
+
x . We get, suppressing the explicit time dependence
|
| 693 |
+
(by taking, e.g.,
|
| 694 |
+
0
|
| 695 |
+
t =
|
| 696 |
+
):
|
| 697 |
+
(8)
|
| 698 |
+
( )
|
| 699 |
+
(
|
| 700 |
+
)
|
| 701 |
+
†
|
| 702 |
+
1
|
| 703 |
+
0
|
| 704 |
+
i
|
| 705 |
+
i
|
| 706 |
+
i
|
| 707 |
+
i
|
| 708 |
+
A
|
| 709 |
+
A
|
| 710 |
+
A
|
| 711 |
+
A a
|
| 712 |
+
Ψ
|
| 713 |
+
=
|
| 714 |
+
=
|
| 715 |
+
=
|
| 716 |
+
p
|
| 717 |
+
p
|
| 718 |
+
p
|
| 719 |
+
x
|
| 720 |
+
p
|
| 721 |
+
|
| 722 |
+
|
| 723 |
+
|
| 724 |
+
|
| 725 |
+
|
| 726 |
+
|
| 727 |
+
|
| 728 |
+
|
| 729 |
+
|
| 730 |
+
|
| 731 |
+
|
| 732 |
+
(
|
| 733 |
+
)
|
| 734 |
+
( )
|
| 735 |
+
( )
|
| 736 |
+
(
|
| 737 |
+
)
|
| 738 |
+
( )
|
| 739 |
+
( )
|
| 740 |
+
(
|
| 741 |
+
)
|
| 742 |
+
3
|
| 743 |
+
0
|
| 744 |
+
0
|
| 745 |
+
3/2
|
| 746 |
+
1
|
| 747 |
+
1
|
| 748 |
+
2
|
| 749 |
+
2
|
| 750 |
+
i
|
| 751 |
+
i
|
| 752 |
+
i
|
| 753 |
+
i
|
| 754 |
+
i
|
| 755 |
+
E A
|
| 756 |
+
A
|
| 757 |
+
A
|
| 758 |
+
e
|
| 759 |
+
d x
|
| 760 |
+
A
|
| 761 |
+
E
|
| 762 |
+
δ
|
| 763 |
+
δ
|
| 764 |
+
π
|
| 765 |
+
⋅
|
| 766 |
+
⎛
|
| 767 |
+
⎞
|
| 768 |
+
=
|
| 769 |
+
Ψ
|
| 770 |
+
−
|
| 771 |
+
Ψ
|
| 772 |
+
⎜
|
| 773 |
+
⎟
|
| 774 |
+
⎝
|
| 775 |
+
⎠
|
| 776 |
+
∫
|
| 777 |
+
p x
|
| 778 |
+
p
|
| 779 |
+
p
|
| 780 |
+
x
|
| 781 |
+
x
|
| 782 |
+
x
|
| 783 |
+
x
|
| 784 |
+
|
| 785 |
+
|
| 786 |
+
|
| 787 |
+
where:
|
| 788 |
+
( )
|
| 789 |
+
(
|
| 790 |
+
)
|
| 791 |
+
( )
|
| 792 |
+
0
|
| 793 |
+
0
|
| 794 |
+
0
|
| 795 |
+
i
|
| 796 |
+
i
|
| 797 |
+
A
|
| 798 |
+
A
|
| 799 |
+
Ψ ≡ Ψ
|
| 800 |
+
⋅
|
| 801 |
+
≡
|
| 802 |
+
⋅
|
| 803 |
+
is the vacuum field wave functional which is
|
| 804 |
+
complex valued and not a function of x , the argument of A, despite its
|
| 805 |
+
notational presence above (to distinguish between position and momentum
|
| 806 |
+
field representations).
|
| 807 |
+
So:
|
| 808 |
+
(9)
|
| 809 |
+
( )
|
| 810 |
+
(
|
| 811 |
+
)
|
| 812 |
+
(
|
| 813 |
+
)
|
| 814 |
+
( )
|
| 815 |
+
(
|
| 816 |
+
)
|
| 817 |
+
( )
|
| 818 |
+
(
|
| 819 |
+
)
|
| 820 |
+
( )
|
| 821 |
+
0
|
| 822 |
+
0
|
| 823 |
+
1
|
| 824 |
+
2
|
| 825 |
+
i
|
| 826 |
+
i
|
| 827 |
+
i
|
| 828 |
+
i
|
| 829 |
+
i
|
| 830 |
+
A
|
| 831 |
+
A
|
| 832 |
+
E A
|
| 833 |
+
A
|
| 834 |
+
A
|
| 835 |
+
E
|
| 836 |
+
δ
|
| 837 |
+
δ
|
| 838 |
+
⎛
|
| 839 |
+
⎞
|
| 840 |
+
Ψ
|
| 841 |
+
⎜
|
| 842 |
+
⎟
|
| 843 |
+
Ψ
|
| 844 |
+
=
|
| 845 |
+
−
|
| 846 |
+
Ψ
|
| 847 |
+
−
|
| 848 |
+
⎜
|
| 849 |
+
⎟
|
| 850 |
+
⎝
|
| 851 |
+
⎠
|
| 852 |
+
�
|
| 853 |
+
�
|
| 854 |
+
p
|
| 855 |
+
p
|
| 856 |
+
p
|
| 857 |
+
x
|
| 858 |
+
x
|
| 859 |
+
p
|
| 860 |
+
x
|
| 861 |
+
p
|
| 862 |
+
,
|
| 863 |
+
where:
|
| 864 |
+
( )
|
| 865 |
+
(
|
| 866 |
+
)
|
| 867 |
+
( )
|
| 868 |
+
3
|
| 869 |
+
3/2
|
| 870 |
+
1
|
| 871 |
+
2
|
| 872 |
+
i
|
| 873 |
+
i
|
| 874 |
+
i
|
| 875 |
+
A
|
| 876 |
+
d p A
|
| 877 |
+
e
|
| 878 |
+
π
|
| 879 |
+
⋅
|
| 880 |
+
≡
|
| 881 |
+
∫
|
| 882 |
+
�
|
| 883 |
+
p x
|
| 884 |
+
x
|
| 885 |
+
p
|
| 886 |
+
, which gives:
|
| 887 |
+
( )
|
| 888 |
+
( )
|
| 889 |
+
/
|
| 890 |
+
i
|
| 891 |
+
i
|
| 892 |
+
i
|
| 893 |
+
A
|
| 894 |
+
A
|
| 895 |
+
e
|
| 896 |
+
δ
|
| 897 |
+
δ
|
| 898 |
+
⋅
|
| 899 |
+
=
|
| 900 |
+
�
|
| 901 |
+
p x
|
| 902 |
+
x
|
| 903 |
+
p
|
| 904 |
+
, and allows us to take
|
| 905 |
+
( )
|
| 906 |
+
iA
|
| 907 |
+
x to be an implicit
|
| 908 |
+
functional of
|
| 909 |
+
( )
|
| 910 |
+
iA�
|
| 911 |
+
p ). Also:
|
| 912 |
+
( )
|
| 913 |
+
( )
|
| 914 |
+
( )
|
| 915 |
+
( )
|
| 916 |
+
(
|
| 917 |
+
)
|
| 918 |
+
( )
|
| 919 |
+
0
|
| 920 |
+
3
|
| 921 |
+
0
|
| 922 |
+
i
|
| 923 |
+
i
|
| 924 |
+
i
|
| 925 |
+
i
|
| 926 |
+
i
|
| 927 |
+
A
|
| 928 |
+
A
|
| 929 |
+
d x
|
| 930 |
+
A
|
| 931 |
+
A
|
| 932 |
+
A
|
| 933 |
+
δ
|
| 934 |
+
δ
|
| 935 |
+
δ
|
| 936 |
+
δ
|
| 937 |
+
δ
|
| 938 |
+
δ
|
| 939 |
+
Ψ
|
| 940 |
+
Ψ
|
| 941 |
+
= ∫
|
| 942 |
+
�
|
| 943 |
+
�
|
| 944 |
+
x
|
| 945 |
+
x
|
| 946 |
+
x
|
| 947 |
+
p
|
| 948 |
+
p
|
| 949 |
+
.
|
| 950 |
+
We need the form of the vacuum wave functional,
|
| 951 |
+
(
|
| 952 |
+
)
|
| 953 |
+
0
|
| 954 |
+
iA
|
| 955 |
+
Ψ
|
| 956 |
+
, which arises from noting:
|
| 957 |
+
(10)a
|
| 958 |
+
ˆ 0
|
| 959 |
+
0
|
| 960 |
+
i
|
| 961 |
+
p
|
| 962 |
+
A a
|
| 963 |
+
=
|
| 964 |
+
|
| 965 |
+
And, using (5) and (7) in this equation, we get:
|
| 966 |
+
(10)b
|
| 967 |
+
( )
|
| 968 |
+
(
|
| 969 |
+
)
|
| 970 |
+
( )
|
| 971 |
+
( )
|
| 972 |
+
( )
|
| 973 |
+
(
|
| 974 |
+
)
|
| 975 |
+
0
|
| 976 |
+
3
|
| 977 |
+
0
|
| 978 |
+
0
|
| 979 |
+
i
|
| 980 |
+
i
|
| 981 |
+
i
|
| 982 |
+
i
|
| 983 |
+
i
|
| 984 |
+
A
|
| 985 |
+
d x e
|
| 986 |
+
E A
|
| 987 |
+
A
|
| 988 |
+
A
|
| 989 |
+
δ
|
| 990 |
+
δ
|
| 991 |
+
−
|
| 992 |
+
⋅ ⎛
|
| 993 |
+
⎞
|
| 994 |
+
Ψ
|
| 995 |
+
⎜
|
| 996 |
+
⎟
|
| 997 |
+
+
|
| 998 |
+
Ψ
|
| 999 |
+
=
|
| 1000 |
+
⎜
|
| 1001 |
+
⎟
|
| 1002 |
+
⎝
|
| 1003 |
+
⎠
|
| 1004 |
+
∫
|
| 1005 |
+
p x
|
| 1006 |
+
p
|
| 1007 |
+
x
|
| 1008 |
+
x
|
| 1009 |
+
x
|
| 1010 |
+
x
|
| 1011 |
+
|
| 1012 |
+
Using, analogous to above,
|
| 1013 |
+
( )
|
| 1014 |
+
(
|
| 1015 |
+
)
|
| 1016 |
+
( )
|
| 1017 |
+
3
|
| 1018 |
+
3/2
|
| 1019 |
+
1
|
| 1020 |
+
2
|
| 1021 |
+
i
|
| 1022 |
+
i
|
| 1023 |
+
i
|
| 1024 |
+
A
|
| 1025 |
+
d x A
|
| 1026 |
+
e
|
| 1027 |
+
π
|
| 1028 |
+
−
|
| 1029 |
+
⋅
|
| 1030 |
+
≡
|
| 1031 |
+
∫
|
| 1032 |
+
�
|
| 1033 |
+
p x
|
| 1034 |
+
p
|
| 1035 |
+
x
|
| 1036 |
+
, we can write:
|
| 1037 |
+
|
| 1038 |
+
6
|
| 1039 |
+
|
| 1040 |
+
(11)
|
| 1041 |
+
|
| 1042 |
+
( )
|
| 1043 |
+
(
|
| 1044 |
+
)
|
| 1045 |
+
0
|
| 1046 |
+
0
|
| 1047 |
+
0
|
| 1048 |
+
i
|
| 1049 |
+
i
|
| 1050 |
+
E A
|
| 1051 |
+
A
|
| 1052 |
+
δ
|
| 1053 |
+
δ
|
| 1054 |
+
Ψ
|
| 1055 |
+
+
|
| 1056 |
+
−
|
| 1057 |
+
Ψ =
|
| 1058 |
+
�
|
| 1059 |
+
�
|
| 1060 |
+
p
|
| 1061 |
+
p
|
| 1062 |
+
p
|
| 1063 |
+
.
|
| 1064 |
+
So, that finally, the vacuum wave functional: is seen to be:
|
| 1065 |
+
(12)
|
| 1066 |
+
(
|
| 1067 |
+
)
|
| 1068 |
+
( )
|
| 1069 |
+
3
|
| 1070 |
+
0
|
| 1071 |
+
1
|
| 1072 |
+
exp
|
| 1073 |
+
2
|
| 1074 |
+
i
|
| 1075 |
+
i
|
| 1076 |
+
N
|
| 1077 |
+
d p E A
|
| 1078 |
+
A
|
| 1079 |
+
⎛
|
| 1080 |
+
⎞
|
| 1081 |
+
Ψ =
|
| 1082 |
+
−
|
| 1083 |
+
⎜
|
| 1084 |
+
⎟
|
| 1085 |
+
⎝
|
| 1086 |
+
⎠
|
| 1087 |
+
∫
|
| 1088 |
+
�
|
| 1089 |
+
�
|
| 1090 |
+
p
|
| 1091 |
+
-p
|
| 1092 |
+
p
|
| 1093 |
+
|
| 1094 |
+
where we drop its
|
| 1095 |
+
( )
|
| 1096 |
+
iA
|
| 1097 |
+
x dependence on Ψ0 because we are here
|
| 1098 |
+
displaying its implicit dependence on
|
| 1099 |
+
( )
|
| 1100 |
+
iA�
|
| 1101 |
+
p and N is the
|
| 1102 |
+
normalization of the wave functional.
|
| 1103 |
+
|
| 1104 |
+
|
| 1105 |
+
Now, we can get the wave functional of the ideal single photon of momentum
|
| 1106 |
+
p by substituting (12) in (9), ignoring the normalization of the wave-functional:
|
| 1107 |
+
(13)
|
| 1108 |
+
|
| 1109 |
+
|
| 1110 |
+
( )
|
| 1111 |
+
(
|
| 1112 |
+
)
|
| 1113 |
+
(
|
| 1114 |
+
)
|
| 1115 |
+
( )
|
| 1116 |
+
3
|
| 1117 |
+
1
|
| 1118 |
+
2
|
| 1119 |
+
2
|
| 1120 |
+
i
|
| 1121 |
+
i
|
| 1122 |
+
d
|
| 1123 |
+
A
|
| 1124 |
+
p
|
| 1125 |
+
i
|
| 1126 |
+
e
|
| 1127 |
+
A
|
| 1128 |
+
A
|
| 1129 |
+
2
|
| 1130 |
+
−
|
| 1131 |
+
Ψ
|
| 1132 |
+
=
|
| 1133 |
+
∫
|
| 1134 |
+
−
|
| 1135 |
+
�
|
| 1136 |
+
p
|
| 1137 |
+
p
|
| 1138 |
+
p
|
| 1139 |
+
x
|
| 1140 |
+
p
|
| 1141 |
+
p
|
| 1142 |
+
,
|
| 1143 |
+
|
| 1144 |
+
|
| 1145 |
+
where we used the fact that ( )
|
| 1146 |
+
A x is real implies
|
| 1147 |
+
( )
|
| 1148 |
+
(
|
| 1149 |
+
)
|
| 1150 |
+
*
|
| 1151 |
+
A
|
| 1152 |
+
A
|
| 1153 |
+
=
|
| 1154 |
+
−
|
| 1155 |
+
�
|
| 1156 |
+
�
|
| 1157 |
+
p
|
| 1158 |
+
p .
|
| 1159 |
+
|
| 1160 |
+
From this, we get the probability of finding the field in a state with a Fourier
|
| 1161 |
+
transform in a small region of functions space
|
| 1162 |
+
i
|
| 1163 |
+
DA� near
|
| 1164 |
+
( )
|
| 1165 |
+
iA�
|
| 1166 |
+
p is:
|
| 1167 |
+
(14)
|
| 1168 |
+
( )
|
| 1169 |
+
(
|
| 1170 |
+
)
|
| 1171 |
+
(
|
| 1172 |
+
)
|
| 1173 |
+
( )
|
| 1174 |
+
( )
|
| 1175 |
+
3
|
| 1176 |
+
2
|
| 1177 |
+
2
|
| 1178 |
+
2
|
| 1179 |
+
i
|
| 1180 |
+
d
|
| 1181 |
+
i
|
| 1182 |
+
i
|
| 1183 |
+
i
|
| 1184 |
+
p
|
| 1185 |
+
A
|
| 1186 |
+
p
|
| 1187 |
+
P A
|
| 1188 |
+
A
|
| 1189 |
+
A
|
| 1190 |
+
e
|
| 1191 |
+
2
|
| 1192 |
+
−∫
|
| 1193 |
+
= Ψ
|
| 1194 |
+
=
|
| 1195 |
+
�
|
| 1196 |
+
�
|
| 1197 |
+
p
|
| 1198 |
+
p
|
| 1199 |
+
p
|
| 1200 |
+
p
|
| 1201 |
+
p
|
| 1202 |
+
.
|
| 1203 |
+
|
| 1204 |
+
We need to find the magnitude of
|
| 1205 |
+
( )
|
| 1206 |
+
iA
|
| 1207 |
+
x , or equivalently the “energy”
|
| 1208 |
+
,
|
| 1209 |
+
2
|
| 1210 |
+
A , that is the most likely.14 Parseval’s theorem tells us that the “energy”
|
| 1211 |
+
spectral density of a spatial function
|
| 1212 |
+
( )
|
| 1213 |
+
iA
|
| 1214 |
+
x is
|
| 1215 |
+
( )
|
| 1216 |
+
( )
|
| 1217 |
+
2
|
| 1218 |
+
i
|
| 1219 |
+
i
|
| 1220 |
+
D
|
| 1221 |
+
A
|
| 1222 |
+
≡ �
|
| 1223 |
+
p
|
| 1224 |
+
p
|
| 1225 |
+
, so in these
|
| 1226 |
+
terms, (14) can be recast as:
|
| 1227 |
+
(15)
|
| 1228 |
+
|
| 1229 |
+
(
|
| 1230 |
+
)
|
| 1231 |
+
( )
|
| 1232 |
+
( )
|
| 1233 |
+
(
|
| 1234 |
+
)
|
| 1235 |
+
(
|
| 1236 |
+
)
|
| 1237 |
+
( ) 3
|
| 1238 |
+
2
|
| 1239 |
+
2
|
| 1240 |
+
2
|
| 1241 |
+
i
|
| 1242 |
+
i
|
| 1243 |
+
i
|
| 1244 |
+
D
|
| 1245 |
+
d p
|
| 1246 |
+
i
|
| 1247 |
+
D
|
| 1248 |
+
D
|
| 1249 |
+
P D
|
| 1250 |
+
e
|
| 1251 |
+
A
|
| 1252 |
+
−∫
|
| 1253 |
+
=
|
| 1254 |
+
+
|
| 1255 |
+
= Ψ p
|
| 1256 |
+
p
|
| 1257 |
+
p
|
| 1258 |
+
p
|
| 1259 |
+
-p
|
| 1260 |
+
p
|
| 1261 |
+
|
| 1262 |
+
where, for the multiplicative factor, we have replaced D by the
|
| 1263 |
+
given sum to make explicit the reflective symmetry of D in p ,15,16
|
| 1264 |
+
which we need to see the consequences of. (Note: such a
|
| 1265 |
+
replacement does not change anything in the integral in the
|
| 1266 |
+
exponent).
|
| 1267 |
+
|
| 1268 |
+
We need to extremize this probability distribution, so we set the first variation to
|
| 1269 |
+
zero giving:
|
| 1270 |
+
|
| 1271 |
+
14 Note we are here interested in A, not E or B. We want to know the most likely vector potential structure.
|
| 1272 |
+
15 D(p) must be even in p for the autocorrelation function to be positive, as it must be.
|
| 1273 |
+
16 Note: even though, for simplicity, we have set p = (0,0,p), no generality was lost in so doing; so we may
|
| 1274 |
+
at any moment let p point in any direction we like.
|
| 1275 |
+
|
| 1276 |
+
7
|
| 1277 |
+
|
| 1278 |
+
(16)
|
| 1279 |
+
|
| 1280 |
+
( )
|
| 1281 |
+
(
|
| 1282 |
+
)
|
| 1283 |
+
( )
|
| 1284 |
+
( )
|
| 1285 |
+
(
|
| 1286 |
+
)
|
| 1287 |
+
(
|
| 1288 |
+
)
|
| 1289 |
+
3
|
| 1290 |
+
2
|
| 1291 |
+
Dd p
|
| 1292 |
+
P D
|
| 1293 |
+
D
|
| 1294 |
+
D
|
| 1295 |
+
e
|
| 1296 |
+
D
|
| 1297 |
+
D
|
| 1298 |
+
δ
|
| 1299 |
+
δ
|
| 1300 |
+
δ
|
| 1301 |
+
δ
|
| 1302 |
+
−
|
| 1303 |
+
⎛
|
| 1304 |
+
⎞
|
| 1305 |
+
+
|
| 1306 |
+
∫
|
| 1307 |
+
∝
|
| 1308 |
+
⎜
|
| 1309 |
+
⎟
|
| 1310 |
+
⎜
|
| 1311 |
+
⎟
|
| 1312 |
+
⎝
|
| 1313 |
+
⎠
|
| 1314 |
+
p
|
| 1315 |
+
p
|
| 1316 |
+
p
|
| 1317 |
+
-p
|
| 1318 |
+
p
|
| 1319 |
+
|
| 1320 |
+
|
| 1321 |
+
|
| 1322 |
+
|
| 1323 |
+
|
| 1324 |
+
|
| 1325 |
+
|
| 1326 |
+
|
| 1327 |
+
|
| 1328 |
+
|
| 1329 |
+
(
|
| 1330 |
+
)
|
| 1331 |
+
(
|
| 1332 |
+
)
|
| 1333 |
+
(
|
| 1334 |
+
)
|
| 1335 |
+
( )
|
| 1336 |
+
3
|
| 1337 |
+
3
|
| 1338 |
+
0
|
| 1339 |
+
2
|
| 1340 |
+
p Dd p
|
| 1341 |
+
Dd p
|
| 1342 |
+
e
|
| 1343 |
+
D
|
| 1344 |
+
e
|
| 1345 |
+
δ
|
| 1346 |
+
δ
|
| 1347 |
+
−
|
| 1348 |
+
−
|
| 1349 |
+
−
|
| 1350 |
+
+
|
| 1351 |
+
+
|
| 1352 |
+
∫
|
| 1353 |
+
∫
|
| 1354 |
+
=
|
| 1355 |
+
−
|
| 1356 |
+
=
|
| 1357 |
+
p
|
| 1358 |
+
p
|
| 1359 |
+
p
|
| 1360 |
+
p
|
| 1361 |
+
p
|
| 1362 |
+
p
|
| 1363 |
+
p
|
| 1364 |
+
,
|
| 1365 |
+
where we have dropped the component index, i, to simplify the notation.
|
| 1366 |
+
Thus, it is seen that the most likely energy spectral density is:
|
| 1367 |
+
(17)
|
| 1368 |
+
|
| 1369 |
+
|
| 1370 |
+
( )
|
| 1371 |
+
(
|
| 1372 |
+
)
|
| 1373 |
+
(
|
| 1374 |
+
)
|
| 1375 |
+
(
|
| 1376 |
+
)
|
| 1377 |
+
max
|
| 1378 |
+
2
|
| 1379 |
+
D
|
| 1380 |
+
δ
|
| 1381 |
+
δ
|
| 1382 |
+
−
|
| 1383 |
+
+
|
| 1384 |
+
+
|
| 1385 |
+
=
|
| 1386 |
+
p
|
| 1387 |
+
p
|
| 1388 |
+
p
|
| 1389 |
+
p
|
| 1390 |
+
p
|
| 1391 |
+
p
|
| 1392 |
+
.
|
| 1393 |
+
This result agrees with the obvious fact that the maximum of
|
| 1394 |
+
(
|
| 1395 |
+
)
|
| 1396 |
+
P D occurs when the
|
| 1397 |
+
integral in the exponent is minimal and the multiplicative factor term is maximal, for at
|
| 1398 |
+
the
|
| 1399 |
+
= ±
|
| 1400 |
+
p
|
| 1401 |
+
p , the factor is infinite, while the exponent is finite.
|
| 1402 |
+
|
| 1403 |
+
Using (17) gives the autocorrelation function:17
|
| 1404 |
+
(18)
|
| 1405 |
+
|
| 1406 |
+
|
| 1407 |
+
3
|
| 1408 |
+
max
|
| 1409 |
+
cos
|
| 1410 |
+
( )
|
| 1411 |
+
[ ( ) (
|
| 1412 |
+
)]
|
| 1413 |
+
( )
|
| 1414 |
+
i
|
| 1415 |
+
AA
|
| 1416 |
+
R
|
| 1417 |
+
A
|
| 1418 |
+
A
|
| 1419 |
+
D
|
| 1420 |
+
e
|
| 1421 |
+
d p
|
| 1422 |
+
∞
|
| 1423 |
+
−∞
|
| 1424 |
+
⋅
|
| 1425 |
+
⋅
|
| 1426 |
+
=
|
| 1427 |
+
+
|
| 1428 |
+
=
|
| 1429 |
+
=
|
| 1430 |
+
∫
|
| 1431 |
+
E
|
| 1432 |
+
p x
|
| 1433 |
+
p x
|
| 1434 |
+
x
|
| 1435 |
+
y
|
| 1436 |
+
y
|
| 1437 |
+
x
|
| 1438 |
+
p
|
| 1439 |
+
p
|
| 1440 |
+
.
|
| 1441 |
+
|
| 1442 |
+
Hence, we see the strong sinusoidal dependence is present in the stochastic A-
|
| 1443 |
+
field that characterizes a single (ideal) photon.
|
| 1444 |
+
N-Photon Wavefunctionals
|
| 1445 |
+
|
| 1446 |
+
Extending what we did in equation (8), and in analogy to the generation of the
|
| 1447 |
+
energy eigenstate wave functions for the harmonic oscillator in ordinary quantum
|
| 1448 |
+
mechanics,18 we construct the wavefunctional corresponding to n photons: 19
|
| 1449 |
+
(19)
|
| 1450 |
+
|
| 1451 |
+
( )
|
| 1452 |
+
(
|
| 1453 |
+
)
|
| 1454 |
+
(
|
| 1455 |
+
)
|
| 1456 |
+
†
|
| 1457 |
+
0
|
| 1458 |
+
n
|
| 1459 |
+
i
|
| 1460 |
+
i
|
| 1461 |
+
i
|
| 1462 |
+
i
|
| 1463 |
+
n
|
| 1464 |
+
A
|
| 1465 |
+
A n
|
| 1466 |
+
A n
|
| 1467 |
+
A
|
| 1468 |
+
a
|
| 1469 |
+
Ψ
|
| 1470 |
+
=
|
| 1471 |
+
=
|
| 1472 |
+
=
|
| 1473 |
+
p
|
| 1474 |
+
p
|
| 1475 |
+
p
|
| 1476 |
+
x
|
| 1477 |
+
p
|
| 1478 |
+
,
|
| 1479 |
+
Substituting (7) and generalizing from (8):
|
| 1480 |
+
(20)
|
| 1481 |
+
( )
|
| 1482 |
+
(
|
| 1483 |
+
)
|
| 1484 |
+
(
|
| 1485 |
+
)
|
| 1486 |
+
(
|
| 1487 |
+
)
|
| 1488 |
+
( )
|
| 1489 |
+
( )
|
| 1490 |
+
3
|
| 1491 |
+
3 /2
|
| 1492 |
+
/2
|
| 1493 |
+
1
|
| 1494 |
+
1
|
| 1495 |
+
ˆ
|
| 1496 |
+
0
|
| 1497 |
+
2
|
| 1498 |
+
2
|
| 1499 |
+
n
|
| 1500 |
+
i
|
| 1501 |
+
i
|
| 1502 |
+
i
|
| 1503 |
+
i
|
| 1504 |
+
n
|
| 1505 |
+
n
|
| 1506 |
+
i
|
| 1507 |
+
A
|
| 1508 |
+
A
|
| 1509 |
+
e
|
| 1510 |
+
E A
|
| 1511 |
+
d x
|
| 1512 |
+
A
|
| 1513 |
+
E
|
| 1514 |
+
δ
|
| 1515 |
+
δ
|
| 1516 |
+
π
|
| 1517 |
+
⋅
|
| 1518 |
+
⎛
|
| 1519 |
+
⎞
|
| 1520 |
+
⎛
|
| 1521 |
+
⎞
|
| 1522 |
+
Ψ
|
| 1523 |
+
=
|
| 1524 |
+
−
|
| 1525 |
+
⎜
|
| 1526 |
+
⎟
|
| 1527 |
+
⎜
|
| 1528 |
+
⎟
|
| 1529 |
+
⎜
|
| 1530 |
+
⎟
|
| 1531 |
+
⎝
|
| 1532 |
+
⎠
|
| 1533 |
+
⎝
|
| 1534 |
+
⎠
|
| 1535 |
+
∫
|
| 1536 |
+
p x
|
| 1537 |
+
np
|
| 1538 |
+
p
|
| 1539 |
+
p
|
| 1540 |
+
x
|
| 1541 |
+
x
|
| 1542 |
+
x
|
| 1543 |
+
|
| 1544 |
+
|
| 1545 |
+
Note: we will need to use:
|
| 1546 |
+
( )
|
| 1547 |
+
( )
|
| 1548 |
+
i
|
| 1549 |
+
A
|
| 1550 |
+
e
|
| 1551 |
+
A
|
| 1552 |
+
δ
|
| 1553 |
+
δ
|
| 1554 |
+
−
|
| 1555 |
+
⋅
|
| 1556 |
+
=
|
| 1557 |
+
�
|
| 1558 |
+
p x
|
| 1559 |
+
p
|
| 1560 |
+
x
|
| 1561 |
+
|
| 1562 |
+
We have already done
|
| 1563 |
+
0
|
| 1564 |
+
n =
|
| 1565 |
+
and
|
| 1566 |
+
1
|
| 1567 |
+
n = case; we now calculate the next three cases (see
|
| 1568 |
+
Appendix A). As a result, we can write the wavefunctionals for 0,1,2, 3 and 4 photons
|
| 1569 |
+
(leaving aside complicating multiplicative factors):
|
| 1570 |
+
(21)
|
| 1571 |
+
|
| 1572 |
+
( )
|
| 1573 |
+
(
|
| 1574 |
+
)
|
| 1575 |
+
( )
|
| 1576 |
+
3
|
| 1577 |
+
1
|
| 1578 |
+
2
|
| 1579 |
+
0
|
| 1580 |
+
iA
|
| 1581 |
+
i
|
| 1582 |
+
d p
|
| 1583 |
+
e
|
| 1584 |
+
A
|
| 1585 |
+
2
|
| 1586 |
+
−
|
| 1587 |
+
Ψ
|
| 1588 |
+
∝
|
| 1589 |
+
∫ p
|
| 1590 |
+
p
|
| 1591 |
+
x
|
| 1592 |
+
|
| 1593 |
+
|
| 1594 |
+
17 In relation to conventional notation, we have:
|
| 1595 |
+
3
|
| 1596 |
+
( )
|
| 1597 |
+
( )
|
| 1598 |
+
( )
|
| 1599 |
+
( )
|
| 1600 |
+
AA
|
| 1601 |
+
A
|
| 1602 |
+
i
|
| 1603 |
+
A
|
| 1604 |
+
A
|
| 1605 |
+
A
|
| 1606 |
+
D
|
| 1607 |
+
S
|
| 1608 |
+
R
|
| 1609 |
+
x e
|
| 1610 |
+
d x
|
| 1611 |
+
R
|
| 1612 |
+
−
|
| 1613 |
+
−∞
|
| 1614 |
+
⋅
|
| 1615 |
+
∞
|
| 1616 |
+
≡
|
| 1617 |
+
=
|
| 1618 |
+
=
|
| 1619 |
+
∫
|
| 1620 |
+
�
|
| 1621 |
+
p x
|
| 1622 |
+
p
|
| 1623 |
+
p
|
| 1624 |
+
p .
|
| 1625 |
+
18 The analogy is fundamentally:
|
| 1626 |
+
( )
|
| 1627 |
+
( )
|
| 1628 |
+
,
|
| 1629 |
+
x
|
| 1630 |
+
A x
|
| 1631 |
+
p
|
| 1632 |
+
A p
|
| 1633 |
+
↔
|
| 1634 |
+
↔ �
|
| 1635 |
+
|
| 1636 |
+
19 Note that the Fourier transform of the general energy eigenstate, is proportional to a state with the exact
|
| 1637 |
+
same formal structure except with x replaced by p, thus in some extended sense it is also an eigenstate of
|
| 1638 |
+
the Fourier operator.
|
| 1639 |
+
|
| 1640 |
+
8
|
| 1641 |
+
|
| 1642 |
+
(22)
|
| 1643 |
+
|
| 1644 |
+
( )
|
| 1645 |
+
(
|
| 1646 |
+
)
|
| 1647 |
+
(
|
| 1648 |
+
)
|
| 1649 |
+
( )
|
| 1650 |
+
3
|
| 1651 |
+
1
|
| 1652 |
+
2
|
| 1653 |
+
2
|
| 1654 |
+
i
|
| 1655 |
+
i
|
| 1656 |
+
d
|
| 1657 |
+
A
|
| 1658 |
+
p
|
| 1659 |
+
i
|
| 1660 |
+
e
|
| 1661 |
+
A
|
| 1662 |
+
A
|
| 1663 |
+
2
|
| 1664 |
+
−
|
| 1665 |
+
Ψ
|
| 1666 |
+
∝
|
| 1667 |
+
∫
|
| 1668 |
+
−
|
| 1669 |
+
�
|
| 1670 |
+
p
|
| 1671 |
+
p
|
| 1672 |
+
p
|
| 1673 |
+
x
|
| 1674 |
+
p
|
| 1675 |
+
p
|
| 1676 |
+
|
| 1677 |
+
(23)
|
| 1678 |
+
|
| 1679 |
+
( )
|
| 1680 |
+
(
|
| 1681 |
+
)
|
| 1682 |
+
(
|
| 1683 |
+
)
|
| 1684 |
+
(
|
| 1685 |
+
)
|
| 1686 |
+
(
|
| 1687 |
+
)
|
| 1688 |
+
(
|
| 1689 |
+
)
|
| 1690 |
+
( )
|
| 1691 |
+
3
|
| 1692 |
+
1
|
| 1693 |
+
2
|
| 1694 |
+
2
|
| 1695 |
+
2
|
| 1696 |
+
2
|
| 1697 |
+
2
|
| 1698 |
+
iA
|
| 1699 |
+
d p
|
| 1700 |
+
i
|
| 1701 |
+
i
|
| 1702 |
+
A
|
| 1703 |
+
e
|
| 1704 |
+
A
|
| 1705 |
+
δ
|
| 1706 |
+
2
|
| 1707 |
+
−
|
| 1708 |
+
Ψ
|
| 1709 |
+
∝
|
| 1710 |
+
−
|
| 1711 |
+
−
|
| 1712 |
+
∫
|
| 1713 |
+
�
|
| 1714 |
+
p
|
| 1715 |
+
p
|
| 1716 |
+
2p
|
| 1717 |
+
x
|
| 1718 |
+
p
|
| 1719 |
+
p
|
| 1720 |
+
p
|
| 1721 |
+
p
|
| 1722 |
+
|
| 1723 |
+
(24)
|
| 1724 |
+
|
| 1725 |
+
( )
|
| 1726 |
+
(
|
| 1727 |
+
)
|
| 1728 |
+
(
|
| 1729 |
+
)
|
| 1730 |
+
(
|
| 1731 |
+
)
|
| 1732 |
+
(
|
| 1733 |
+
)
|
| 1734 |
+
(
|
| 1735 |
+
) (
|
| 1736 |
+
)
|
| 1737 |
+
(
|
| 1738 |
+
)
|
| 1739 |
+
( )
|
| 1740 |
+
3
|
| 1741 |
+
1
|
| 1742 |
+
3
|
| 1743 |
+
2
|
| 1744 |
+
2
|
| 1745 |
+
4
|
| 1746 |
+
2
|
| 1747 |
+
3
|
| 1748 |
+
2
|
| 1749 |
+
iA
|
| 1750 |
+
p
|
| 1751 |
+
i
|
| 1752 |
+
i
|
| 1753 |
+
i
|
| 1754 |
+
d
|
| 1755 |
+
e
|
| 1756 |
+
A
|
| 1757 |
+
A
|
| 1758 |
+
A
|
| 1759 |
+
δ
|
| 1760 |
+
2
|
| 1761 |
+
−
|
| 1762 |
+
Ψ
|
| 1763 |
+
∝
|
| 1764 |
+
−
|
| 1765 |
+
−
|
| 1766 |
+
−
|
| 1767 |
+
∫
|
| 1768 |
+
�
|
| 1769 |
+
�
|
| 1770 |
+
p
|
| 1771 |
+
p
|
| 1772 |
+
3p
|
| 1773 |
+
x
|
| 1774 |
+
p
|
| 1775 |
+
p
|
| 1776 |
+
p
|
| 1777 |
+
p
|
| 1778 |
+
p
|
| 1779 |
+
|
| 1780 |
+
(25)
|
| 1781 |
+
|
| 1782 |
+
( )
|
| 1783 |
+
(
|
| 1784 |
+
)
|
| 1785 |
+
(
|
| 1786 |
+
)
|
| 1787 |
+
(
|
| 1788 |
+
)
|
| 1789 |
+
(
|
| 1790 |
+
)
|
| 1791 |
+
(
|
| 1792 |
+
)
|
| 1793 |
+
(
|
| 1794 |
+
)
|
| 1795 |
+
(
|
| 1796 |
+
)
|
| 1797 |
+
(
|
| 1798 |
+
)
|
| 1799 |
+
( )
|
| 1800 |
+
3
|
| 1801 |
+
1
|
| 1802 |
+
4
|
| 1803 |
+
2
|
| 1804 |
+
2
|
| 1805 |
+
2
|
| 1806 |
+
2
|
| 1807 |
+
2
|
| 1808 |
+
4
|
| 1809 |
+
12
|
| 1810 |
+
2
|
| 1811 |
+
4
|
| 1812 |
+
3
|
| 1813 |
+
2
|
| 1814 |
+
i
|
| 1815 |
+
i
|
| 1816 |
+
i
|
| 1817 |
+
A
|
| 1818 |
+
p
|
| 1819 |
+
i
|
| 1820 |
+
d
|
| 1821 |
+
A
|
| 1822 |
+
e
|
| 1823 |
+
A
|
| 1824 |
+
A
|
| 1825 |
+
δ
|
| 1826 |
+
δ
|
| 1827 |
+
2
|
| 1828 |
+
−
|
| 1829 |
+
⎛
|
| 1830 |
+
⎞
|
| 1831 |
+
−
|
| 1832 |
+
−
|
| 1833 |
+
⎜
|
| 1834 |
+
⎟
|
| 1835 |
+
Ψ
|
| 1836 |
+
∝
|
| 1837 |
+
⎜
|
| 1838 |
+
⎟
|
| 1839 |
+
+
|
| 1840 |
+
⎝
|
| 1841 |
+
⎠
|
| 1842 |
+
∫
|
| 1843 |
+
�
|
| 1844 |
+
�
|
| 1845 |
+
p
|
| 1846 |
+
p
|
| 1847 |
+
4p
|
| 1848 |
+
p
|
| 1849 |
+
p
|
| 1850 |
+
p
|
| 1851 |
+
-p
|
| 1852 |
+
p
|
| 1853 |
+
x
|
| 1854 |
+
p
|
| 1855 |
+
p
|
| 1856 |
+
|
| 1857 |
+
Now, we can drop the ( )
|
| 1858 |
+
δ
|
| 1859 |
+
p terms, as we have obviously chosen
|
| 1860 |
+
0
|
| 1861 |
+
≠
|
| 1862 |
+
p
|
| 1863 |
+
; so, for example,
|
| 1864 |
+
for the 4-photon case we get:
|
| 1865 |
+
(26)
|
| 1866 |
+
|
| 1867 |
+
( )
|
| 1868 |
+
(
|
| 1869 |
+
)
|
| 1870 |
+
(
|
| 1871 |
+
)
|
| 1872 |
+
(
|
| 1873 |
+
)
|
| 1874 |
+
( )
|
| 1875 |
+
3
|
| 1876 |
+
4
|
| 1877 |
+
4
|
| 1878 |
+
1
|
| 1879 |
+
2
|
| 1880 |
+
16
|
| 1881 |
+
iA
|
| 1882 |
+
p
|
| 1883 |
+
i
|
| 1884 |
+
i
|
| 1885 |
+
d
|
| 1886 |
+
e
|
| 1887 |
+
A
|
| 1888 |
+
A
|
| 1889 |
+
2
|
| 1890 |
+
−
|
| 1891 |
+
Ψ
|
| 1892 |
+
∝
|
| 1893 |
+
−
|
| 1894 |
+
∫
|
| 1895 |
+
�
|
| 1896 |
+
p
|
| 1897 |
+
p
|
| 1898 |
+
4p
|
| 1899 |
+
x
|
| 1900 |
+
p
|
| 1901 |
+
p
|
| 1902 |
+
|
| 1903 |
+
(
|
| 1904 |
+
0
|
| 1905 |
+
≠
|
| 1906 |
+
p
|
| 1907 |
+
)
|
| 1908 |
+
|
| 1909 |
+
We see the pattern. Using the formal analogy to the ordinary quantum oscillator,20
|
| 1910 |
+
or induction, we can write the first try at the solution as, dropping the component
|
| 1911 |
+
superscript, i, and the multiplicative factors:
|
| 1912 |
+
(27)
|
| 1913 |
+
1st try:
|
| 1914 |
+
( )
|
| 1915 |
+
(
|
| 1916 |
+
)
|
| 1917 |
+
(
|
| 1918 |
+
)
|
| 1919 |
+
( )
|
| 1920 |
+
(
|
| 1921 |
+
)
|
| 1922 |
+
(
|
| 1923 |
+
)
|
| 1924 |
+
(
|
| 1925 |
+
)
|
| 1926 |
+
(
|
| 1927 |
+
)
|
| 1928 |
+
(
|
| 1929 |
+
)
|
| 1930 |
+
3
|
| 1931 |
+
3
|
| 1932 |
+
3
|
| 1933 |
+
2
|
| 1934 |
+
2
|
| 1935 |
+
1
|
| 1936 |
+
2
|
| 1937 |
+
.
|
| 1938 |
+
1
|
| 1939 |
+
i
|
| 1940 |
+
n
|
| 1941 |
+
d
|
| 1942 |
+
d p
|
| 1943 |
+
A
|
| 1944 |
+
p
|
| 1945 |
+
A
|
| 1946 |
+
A
|
| 1947 |
+
n
|
| 1948 |
+
d p
|
| 1949 |
+
n
|
| 1950 |
+
n
|
| 1951 |
+
A
|
| 1952 |
+
e
|
| 1953 |
+
e
|
| 1954 |
+
e
|
| 1955 |
+
A
|
| 1956 |
+
δ
|
| 1957 |
+
δ
|
| 1958 |
+
2
|
| 1959 |
+
−
|
| 1960 |
+
−
|
| 1961 |
+
−
|
| 1962 |
+
−
|
| 1963 |
+
Ψ
|
| 1964 |
+
∝
|
| 1965 |
+
∫
|
| 1966 |
+
∫
|
| 1967 |
+
∫
|
| 1968 |
+
−
|
| 1969 |
+
−
|
| 1970 |
+
�
|
| 1971 |
+
�
|
| 1972 |
+
�
|
| 1973 |
+
p
|
| 1974 |
+
p
|
| 1975 |
+
p
|
| 1976 |
+
p
|
| 1977 |
+
p
|
| 1978 |
+
p
|
| 1979 |
+
p
|
| 1980 |
+
x
|
| 1981 |
+
p
|
| 1982 |
+
|
| 1983 |
+
This first try, however, includes the terms that correspond to the delta functions which, as
|
| 1984 |
+
just stated, we don’t need; so, we write:
|
| 1985 |
+
(28)
|
| 1986 |
+
( )
|
| 1987 |
+
(
|
| 1988 |
+
)
|
| 1989 |
+
( )
|
| 1990 |
+
(
|
| 1991 |
+
)
|
| 1992 |
+
(
|
| 1993 |
+
)
|
| 1994 |
+
(
|
| 1995 |
+
)
|
| 1996 |
+
(
|
| 1997 |
+
)
|
| 1998 |
+
(
|
| 1999 |
+
)
|
| 2000 |
+
(
|
| 2001 |
+
)
|
| 2002 |
+
( )
|
| 2003 |
+
3
|
| 2004 |
+
3
|
| 2005 |
+
1
|
| 2006 |
+
1
|
| 2007 |
+
2
|
| 2008 |
+
2
|
| 2009 |
+
.
|
| 2010 |
+
1
|
| 2011 |
+
2
|
| 2012 |
+
2
|
| 2013 |
+
i
|
| 2014 |
+
i
|
| 2015 |
+
d
|
| 2016 |
+
d
|
| 2017 |
+
A
|
| 2018 |
+
p
|
| 2019 |
+
A
|
| 2020 |
+
p
|
| 2021 |
+
n
|
| 2022 |
+
n
|
| 2023 |
+
n
|
| 2024 |
+
n
|
| 2025 |
+
n
|
| 2026 |
+
A
|
| 2027 |
+
A
|
| 2028 |
+
e
|
| 2029 |
+
e
|
| 2030 |
+
A
|
| 2031 |
+
2
|
| 2032 |
+
2
|
| 2033 |
+
−
|
| 2034 |
+
−
|
| 2035 |
+
∫
|
| 2036 |
+
Ψ
|
| 2037 |
+
∝
|
| 2038 |
+
−
|
| 2039 |
+
−
|
| 2040 |
+
−
|
| 2041 |
+
∫
|
| 2042 |
+
−
|
| 2043 |
+
=
|
| 2044 |
+
�
|
| 2045 |
+
�
|
| 2046 |
+
p
|
| 2047 |
+
p
|
| 2048 |
+
p
|
| 2049 |
+
p
|
| 2050 |
+
p
|
| 2051 |
+
x
|
| 2052 |
+
p
|
| 2053 |
+
p
|
| 2054 |
+
p
|
| 2055 |
+
p
|
| 2056 |
+
|
| 2057 |
+
|
| 2058 |
+
This means the corresponding probability distribution is, dropping constant
|
| 2059 |
+
multiplicative factors:
|
| 2060 |
+
(29)
|
| 2061 |
+
|
| 2062 |
+
(
|
| 2063 |
+
)
|
| 2064 |
+
( )
|
| 2065 |
+
( )
|
| 2066 |
+
( )
|
| 2067 |
+
( )
|
| 2068 |
+
3
|
| 2069 |
+
3
|
| 2070 |
+
2
|
| 2071 |
+
i
|
| 2072 |
+
i
|
| 2073 |
+
d
|
| 2074 |
+
n
|
| 2075 |
+
A
|
| 2076 |
+
p
|
| 2077 |
+
A
|
| 2078 |
+
p
|
| 2079 |
+
n
|
| 2080 |
+
d
|
| 2081 |
+
n
|
| 2082 |
+
A
|
| 2083 |
+
D
|
| 2084 |
+
P
|
| 2085 |
+
D
|
| 2086 |
+
e
|
| 2087 |
+
e
|
| 2088 |
+
2
|
| 2089 |
+
2
|
| 2090 |
+
−
|
| 2091 |
+
−
|
| 2092 |
+
∝
|
| 2093 |
+
=
|
| 2094 |
+
∫
|
| 2095 |
+
∫
|
| 2096 |
+
�
|
| 2097 |
+
p
|
| 2098 |
+
p
|
| 2099 |
+
p
|
| 2100 |
+
p
|
| 2101 |
+
p
|
| 2102 |
+
p
|
| 2103 |
+
p
|
| 2104 |
+
,
|
| 2105 |
+
|
| 2106 |
+
where we introduce
|
| 2107 |
+
( )
|
| 2108 |
+
( )
|
| 2109 |
+
(
|
| 2110 |
+
)
|
| 2111 |
+
(
|
| 2112 |
+
) / 2
|
| 2113 |
+
D
|
| 2114 |
+
D
|
| 2115 |
+
D
|
| 2116 |
+
≡
|
| 2117 |
+
+
|
| 2118 |
+
−
|
| 2119 |
+
p
|
| 2120 |
+
p
|
| 2121 |
+
p
|
| 2122 |
+
to make D’s
|
| 2123 |
+
symmetry in p explicit for the minimization differentiation.
|
| 2124 |
+
Minimizing gives:
|
| 2125 |
+
(30)
|
| 2126 |
+
|
| 2127 |
+
( )
|
| 2128 |
+
(
|
| 2129 |
+
)
|
| 2130 |
+
( )
|
| 2131 |
+
( )
|
| 2132 |
+
(
|
| 2133 |
+
)
|
| 2134 |
+
( )
|
| 2135 |
+
3
|
| 2136 |
+
2
|
| 2137 |
+
d
|
| 2138 |
+
n
|
| 2139 |
+
D
|
| 2140 |
+
np
|
| 2141 |
+
p
|
| 2142 |
+
P
|
| 2143 |
+
D
|
| 2144 |
+
D
|
| 2145 |
+
D
|
| 2146 |
+
D
|
| 2147 |
+
D
|
| 2148 |
+
e
|
| 2149 |
+
δ
|
| 2150 |
+
δ
|
| 2151 |
+
δ
|
| 2152 |
+
δ
|
| 2153 |
+
−
|
| 2154 |
+
⎛
|
| 2155 |
+
⎞
|
| 2156 |
+
+
|
| 2157 |
+
−
|
| 2158 |
+
⎛
|
| 2159 |
+
⎞
|
| 2160 |
+
⎜
|
| 2161 |
+
⎟
|
| 2162 |
+
∝
|
| 2163 |
+
⎜
|
| 2164 |
+
⎟
|
| 2165 |
+
⎜
|
| 2166 |
+
⎟
|
| 2167 |
+
⎝
|
| 2168 |
+
⎠
|
| 2169 |
+
⎝
|
| 2170 |
+
∫
|
| 2171 |
+
⎠
|
| 2172 |
+
p
|
| 2173 |
+
p
|
| 2174 |
+
p
|
| 2175 |
+
p
|
| 2176 |
+
p
|
| 2177 |
+
p
|
| 2178 |
+
|
| 2179 |
+
|
| 2180 |
+
( )
|
| 2181 |
+
(
|
| 2182 |
+
)
|
| 2183 |
+
(
|
| 2184 |
+
)
|
| 2185 |
+
( )
|
| 2186 |
+
( )
|
| 2187 |
+
( )
|
| 2188 |
+
3
|
| 2189 |
+
3
|
| 2190 |
+
1
|
| 2191 |
+
0
|
| 2192 |
+
2
|
| 2193 |
+
n
|
| 2194 |
+
D
|
| 2195 |
+
D
|
| 2196 |
+
n
|
| 2197 |
+
d p
|
| 2198 |
+
d
|
| 2199 |
+
n
|
| 2200 |
+
p
|
| 2201 |
+
e
|
| 2202 |
+
e
|
| 2203 |
+
nD
|
| 2204 |
+
D
|
| 2205 |
+
δ
|
| 2206 |
+
δ
|
| 2207 |
+
−
|
| 2208 |
+
−
|
| 2209 |
+
−
|
| 2210 |
+
−
|
| 2211 |
+
+
|
| 2212 |
+
+
|
| 2213 |
+
⎛
|
| 2214 |
+
⎞
|
| 2215 |
+
−
|
| 2216 |
+
∫
|
| 2217 |
+
∫
|
| 2218 |
+
=
|
| 2219 |
+
=
|
| 2220 |
+
⎜
|
| 2221 |
+
⎟
|
| 2222 |
+
⎝
|
| 2223 |
+
⎠
|
| 2224 |
+
p
|
| 2225 |
+
p
|
| 2226 |
+
p
|
| 2227 |
+
p
|
| 2228 |
+
p
|
| 2229 |
+
p
|
| 2230 |
+
p
|
| 2231 |
+
p
|
| 2232 |
+
p
|
| 2233 |
+
p
|
| 2234 |
+
p
|
| 2235 |
+
|
| 2236 |
+
which implies, dropping the explicit separation of D in the first term:
|
| 2237 |
+
|
| 2238 |
+
20 The Fourier transform of the energy eigenstates (
|
| 2239 |
+
2
|
| 2240 |
+
exp(
|
| 2241 |
+
)
|
| 2242 |
+
/ 2)
|
| 2243 |
+
(
|
| 2244 |
+
n
|
| 2245 |
+
n
|
| 2246 |
+
x
|
| 2247 |
+
H
|
| 2248 |
+
x
|
| 2249 |
+
ψ
|
| 2250 |
+
=
|
| 2251 |
+
−
|
| 2252 |
+
) in ordinary quantum
|
| 2253 |
+
mechanics,
|
| 2254 |
+
that
|
| 2255 |
+
we
|
| 2256 |
+
use
|
| 2257 |
+
here
|
| 2258 |
+
by
|
| 2259 |
+
analogy
|
| 2260 |
+
is:
|
| 2261 |
+
(
|
| 2262 |
+
)
|
| 2263 |
+
2
|
| 2264 |
+
2
|
| 2265 |
+
exp(
|
| 2266 |
+
/
|
| 2267 |
+
( )
|
| 2268 |
+
(
|
| 2269 |
+
x
|
| 2270 |
+
2
|
| 2271 |
+
/
|
| 2272 |
+
)
|
| 2273 |
+
e p(
|
| 2274 |
+
)
|
| 2275 |
+
)
|
| 2276 |
+
n
|
| 2277 |
+
n
|
| 2278 |
+
n
|
| 2279 |
+
n
|
| 2280 |
+
p
|
| 2281 |
+
p
|
| 2282 |
+
p
|
| 2283 |
+
i
|
| 2284 |
+
d
|
| 2285 |
+
dp
|
| 2286 |
+
ψ
|
| 2287 |
+
=
|
| 2288 |
+
−
|
| 2289 |
+
|
| 2290 |
+
Note:
|
| 2291 |
+
2
|
| 2292 |
+
2
|
| 2293 |
+
exp
|
| 2294 |
+
( )
|
| 2295 |
+
(
|
| 2296 |
+
( 1)
|
| 2297 |
+
exp(
|
| 2298 |
+
/
|
| 2299 |
+
)
|
| 2300 |
+
)
|
| 2301 |
+
n
|
| 2302 |
+
n
|
| 2303 |
+
n
|
| 2304 |
+
n
|
| 2305 |
+
H
|
| 2306 |
+
x
|
| 2307 |
+
x
|
| 2308 |
+
x
|
| 2309 |
+
x
|
| 2310 |
+
d
|
| 2311 |
+
d
|
| 2312 |
+
= −
|
| 2313 |
+
−
|
| 2314 |
+
.
|
| 2315 |
+
|
| 2316 |
+
9
|
| 2317 |
+
|
| 2318 |
+
(31)
|
| 2319 |
+
|
| 2320 |
+
( )
|
| 2321 |
+
(
|
| 2322 |
+
)
|
| 2323 |
+
(
|
| 2324 |
+
)
|
| 2325 |
+
( )
|
| 2326 |
+
1
|
| 2327 |
+
2
|
| 2328 |
+
n
|
| 2329 |
+
n
|
| 2330 |
+
nD
|
| 2331 |
+
D
|
| 2332 |
+
δ
|
| 2333 |
+
δ
|
| 2334 |
+
−
|
| 2335 |
+
−
|
| 2336 |
+
+
|
| 2337 |
+
+
|
| 2338 |
+
⎛
|
| 2339 |
+
⎞ =
|
| 2340 |
+
⎜
|
| 2341 |
+
⎟
|
| 2342 |
+
⎝
|
| 2343 |
+
⎠
|
| 2344 |
+
p
|
| 2345 |
+
p
|
| 2346 |
+
p
|
| 2347 |
+
p
|
| 2348 |
+
p
|
| 2349 |
+
p
|
| 2350 |
+
p
|
| 2351 |
+
|
| 2352 |
+
So we have:
|
| 2353 |
+
(32)
|
| 2354 |
+
|
| 2355 |
+
( )
|
| 2356 |
+
(
|
| 2357 |
+
)
|
| 2358 |
+
(
|
| 2359 |
+
)
|
| 2360 |
+
2
|
| 2361 |
+
D
|
| 2362 |
+
n δ
|
| 2363 |
+
δ
|
| 2364 |
+
⎛
|
| 2365 |
+
⎞
|
| 2366 |
+
−
|
| 2367 |
+
+
|
| 2368 |
+
+
|
| 2369 |
+
=
|
| 2370 |
+
⎜
|
| 2371 |
+
⎟
|
| 2372 |
+
⎝
|
| 2373 |
+
⎠
|
| 2374 |
+
p
|
| 2375 |
+
p
|
| 2376 |
+
p
|
| 2377 |
+
p
|
| 2378 |
+
p
|
| 2379 |
+
p
|
| 2380 |
+
|
| 2381 |
+
|
| 2382 |
+
So n photons have n times the energy spectral density as a single one, but the
|
| 2383 |
+
same concentration of that energy into a sinusoidal form. This is a very nice result that
|
| 2384 |
+
agrees with ones intuition; one can think of the field of a photon as mostly having sine-
|
| 2385 |
+
like behavior, but on top of a stochastic background. (Of course, more information can be
|
| 2386 |
+
extracted from the wavefunctional, such as the moments of the distribution.)
|
| 2387 |
+
|
| 2388 |
+
Many-photon Wave-functionals with Different Momenta
|
| 2389 |
+
|
| 2390 |
+
The above formalism is generalizable to the photons of different momenta. The
|
| 2391 |
+
basic principle can be illustrated by the two photon case, one with momentum
|
| 2392 |
+
1p the
|
| 2393 |
+
other with momentum
|
| 2394 |
+
2p .
|
| 2395 |
+
We can extend the general formalism to this case by applying the creation operator twice
|
| 2396 |
+
(
|
| 2397 |
+
)
|
| 2398 |
+
(
|
| 2399 |
+
)
|
| 2400 |
+
†
|
| 2401 |
+
†
|
| 2402 |
+
1
|
| 2403 |
+
2
|
| 2404 |
+
2
|
| 2405 |
+
1
|
| 2406 |
+
,
|
| 2407 |
+
0
|
| 2408 |
+
p
|
| 2409 |
+
p
|
| 2410 |
+
a
|
| 2411 |
+
p
|
| 2412 |
+
a
|
| 2413 |
+
p
|
| 2414 |
+
=
|
| 2415 |
+
); we get, temporarily dropping the factor
|
| 2416 |
+
( )
|
| 2417 |
+
3
|
| 2418 |
+
d p
|
| 2419 |
+
D
|
| 2420 |
+
e
|
| 2421 |
+
−∫ p
|
| 2422 |
+
p
|
| 2423 |
+
:
|
| 2424 |
+
(33)
|
| 2425 |
+
(
|
| 2426 |
+
) (
|
| 2427 |
+
)
|
| 2428 |
+
(
|
| 2429 |
+
)
|
| 2430 |
+
(
|
| 2431 |
+
)
|
| 2432 |
+
(
|
| 2433 |
+
)
|
| 2434 |
+
(
|
| 2435 |
+
)
|
| 2436 |
+
(
|
| 2437 |
+
)
|
| 2438 |
+
(
|
| 2439 |
+
)
|
| 2440 |
+
1
|
| 2441 |
+
2
|
| 2442 |
+
1
|
| 2443 |
+
2
|
| 2444 |
+
1
|
| 2445 |
+
2
|
| 2446 |
+
1
|
| 2447 |
+
2
|
| 2448 |
+
1
|
| 2449 |
+
2
|
| 2450 |
+
1
|
| 2451 |
+
1
|
| 2452 |
+
2
|
| 2453 |
+
*
|
| 2454 |
+
,
|
| 2455 |
+
,
|
| 2456 |
+
,
|
| 2457 |
+
*
|
| 2458 |
+
*
|
| 2459 |
+
1
|
| 2460 |
+
2
|
| 2461 |
+
1
|
| 2462 |
+
2
|
| 2463 |
+
1
|
| 2464 |
+
1
|
| 2465 |
+
2
|
| 2466 |
+
4
|
| 2467 |
+
2
|
| 2468 |
+
4
|
| 2469 |
+
2
|
| 2470 |
+
A
|
| 2471 |
+
A
|
| 2472 |
+
P
|
| 2473 |
+
A
|
| 2474 |
+
A
|
| 2475 |
+
δ
|
| 2476 |
+
ψ
|
| 2477 |
+
ψ
|
| 2478 |
+
δ
|
| 2479 |
+
⎛
|
| 2480 |
+
⎞
|
| 2481 |
+
−
|
| 2482 |
+
+
|
| 2483 |
+
×
|
| 2484 |
+
⎜
|
| 2485 |
+
⎟
|
| 2486 |
+
=
|
| 2487 |
+
∝ ⎜
|
| 2488 |
+
⎟
|
| 2489 |
+
−
|
| 2490 |
+
+
|
| 2491 |
+
⎝
|
| 2492 |
+
⎠
|
| 2493 |
+
p
|
| 2494 |
+
p
|
| 2495 |
+
p
|
| 2496 |
+
p
|
| 2497 |
+
p
|
| 2498 |
+
p
|
| 2499 |
+
p
|
| 2500 |
+
p
|
| 2501 |
+
p
|
| 2502 |
+
p
|
| 2503 |
+
p
|
| 2504 |
+
p
|
| 2505 |
+
p
|
| 2506 |
+
p
|
| 2507 |
+
p
|
| 2508 |
+
p
|
| 2509 |
+
p
|
| 2510 |
+
p
|
| 2511 |
+
p
|
| 2512 |
+
p
|
| 2513 |
+
|
| 2514 |
+
(
|
| 2515 |
+
)(
|
| 2516 |
+
)
|
| 2517 |
+
(
|
| 2518 |
+
)
|
| 2519 |
+
(
|
| 2520 |
+
)
|
| 2521 |
+
(
|
| 2522 |
+
)
|
| 2523 |
+
2
|
| 2524 |
+
2
|
| 2525 |
+
*
|
| 2526 |
+
*
|
| 2527 |
+
1
|
| 2528 |
+
2
|
| 2529 |
+
1
|
| 2530 |
+
2
|
| 2531 |
+
1
|
| 2532 |
+
2
|
| 2533 |
+
1
|
| 2534 |
+
2
|
| 2535 |
+
1
|
| 2536 |
+
2
|
| 2537 |
+
1
|
| 2538 |
+
2
|
| 2539 |
+
1
|
| 2540 |
+
1
|
| 2541 |
+
2
|
| 2542 |
+
8
|
| 2543 |
+
2
|
| 2544 |
+
4
|
| 2545 |
+
D D
|
| 2546 |
+
A A
|
| 2547 |
+
A A
|
| 2548 |
+
δ
|
| 2549 |
+
δ
|
| 2550 |
+
=
|
| 2551 |
+
−
|
| 2552 |
+
+
|
| 2553 |
+
+
|
| 2554 |
+
+
|
| 2555 |
+
+
|
| 2556 |
+
p
|
| 2557 |
+
p
|
| 2558 |
+
p
|
| 2559 |
+
p
|
| 2560 |
+
p
|
| 2561 |
+
p
|
| 2562 |
+
p
|
| 2563 |
+
p
|
| 2564 |
+
p
|
| 2565 |
+
|
| 2566 |
+
|
| 2567 |
+
|
| 2568 |
+
First, we consider the most general and most interesting case (for these idealized
|
| 2569 |
+
photons), which is also the simplest to calculate.
|
| 2570 |
+
Case I:
|
| 2571 |
+
1
|
| 2572 |
+
2
|
| 2573 |
+
≠ −
|
| 2574 |
+
p
|
| 2575 |
+
p .
|
| 2576 |
+
This means the delta functions in (33) are not in play, so we have, in terms of the
|
| 2577 |
+
previously defined D and reinserting the exponential term:
|
| 2578 |
+
(34)
|
| 2579 |
+
|
| 2580 |
+
(
|
| 2581 |
+
)
|
| 2582 |
+
(
|
| 2583 |
+
)
|
| 2584 |
+
(
|
| 2585 |
+
)
|
| 2586 |
+
(
|
| 2587 |
+
)
|
| 2588 |
+
(
|
| 2589 |
+
)
|
| 2590 |
+
( )
|
| 2591 |
+
2
|
| 2592 |
+
3
|
| 2593 |
+
1
|
| 2594 |
+
2
|
| 2595 |
+
2
|
| 2596 |
+
,
|
| 2597 |
+
1
|
| 2598 |
+
2
|
| 2599 |
+
1
|
| 2600 |
+
2
|
| 2601 |
+
1
|
| 2602 |
+
2
|
| 2603 |
+
2
|
| 2604 |
+
,
|
| 2605 |
+
16
|
| 2606 |
+
d
|
| 2607 |
+
D
|
| 2608 |
+
p
|
| 2609 |
+
p
|
| 2610 |
+
p
|
| 2611 |
+
P
|
| 2612 |
+
D p
|
| 2613 |
+
D p
|
| 2614 |
+
D
|
| 2615 |
+
D
|
| 2616 |
+
e
|
| 2617 |
+
−∫
|
| 2618 |
+
∝
|
| 2619 |
+
p
|
| 2620 |
+
p
|
| 2621 |
+
p
|
| 2622 |
+
p
|
| 2623 |
+
p
|
| 2624 |
+
p
|
| 2625 |
+
|
| 2626 |
+
We want:
|
| 2627 |
+
1
|
| 2628 |
+
2
|
| 2629 |
+
,
|
| 2630 |
+
1
|
| 2631 |
+
0
|
| 2632 |
+
p
|
| 2633 |
+
p
|
| 2634 |
+
P
|
| 2635 |
+
D
|
| 2636 |
+
δ
|
| 2637 |
+
δ
|
| 2638 |
+
=
|
| 2639 |
+
and
|
| 2640 |
+
1
|
| 2641 |
+
2
|
| 2642 |
+
,
|
| 2643 |
+
2
|
| 2644 |
+
0
|
| 2645 |
+
p
|
| 2646 |
+
p
|
| 2647 |
+
P
|
| 2648 |
+
D
|
| 2649 |
+
δ
|
| 2650 |
+
δ
|
| 2651 |
+
=
|
| 2652 |
+
.
|
| 2653 |
+
Since this is formally same as calculation previously done, we get:
|
| 2654 |
+
(
|
| 2655 |
+
)
|
| 2656 |
+
(
|
| 2657 |
+
)
|
| 2658 |
+
2
|
| 2659 |
+
i
|
| 2660 |
+
i
|
| 2661 |
+
i
|
| 2662 |
+
i
|
| 2663 |
+
D
|
| 2664 |
+
δ
|
| 2665 |
+
δ
|
| 2666 |
+
−
|
| 2667 |
+
+
|
| 2668 |
+
−
|
| 2669 |
+
=
|
| 2670 |
+
p
|
| 2671 |
+
p
|
| 2672 |
+
p
|
| 2673 |
+
p
|
| 2674 |
+
p
|
| 2675 |
+
. So, as expected, we get one field structure with strong
|
| 2676 |
+
sinusoidal structure of frequency associated with
|
| 2677 |
+
1p and one associated with
|
| 2678 |
+
2p . Note
|
| 2679 |
+
equation (34) and this last result reduce to the same result for the case in which
|
| 2680 |
+
1
|
| 2681 |
+
2
|
| 2682 |
+
≡
|
| 2683 |
+
=
|
| 2684 |
+
p
|
| 2685 |
+
p
|
| 2686 |
+
p ; to see the latter, compare equations (34) and (29). This again verifies our
|
| 2687 |
+
intuition of two photon systems.
|
| 2688 |
+
|
| 2689 |
+
We now move to the second, more limited case.
|
| 2690 |
+
Case II:
|
| 2691 |
+
1
|
| 2692 |
+
2
|
| 2693 |
+
= −
|
| 2694 |
+
p
|
| 2695 |
+
p
|
| 2696 |
+
|
| 2697 |
+
10
|
| 2698 |
+
|
| 2699 |
+
|
| 2700 |
+
Given our analysis in the previous sections, we would expect the two photons
|
| 2701 |
+
might cancel each other out in our (idealized photon) case. To do the calculation, we take
|
| 2702 |
+
the following definitions:
|
| 2703 |
+
1
|
| 2704 |
+
2
|
| 2705 |
+
≡
|
| 2706 |
+
= −
|
| 2707 |
+
p
|
| 2708 |
+
p
|
| 2709 |
+
p ,
|
| 2710 |
+
(
|
| 2711 |
+
) (
|
| 2712 |
+
)
|
| 2713 |
+
( )
|
| 2714 |
+
2
|
| 2715 |
+
2
|
| 2716 |
+
i
|
| 2717 |
+
i
|
| 2718 |
+
i
|
| 2719 |
+
i
|
| 2720 |
+
D
|
| 2721 |
+
D
|
| 2722 |
+
A
|
| 2723 |
+
A
|
| 2724 |
+
A
|
| 2725 |
+
A
|
| 2726 |
+
≡
|
| 2727 |
+
≡
|
| 2728 |
+
=
|
| 2729 |
+
−
|
| 2730 |
+
=
|
| 2731 |
+
p
|
| 2732 |
+
p
|
| 2733 |
+
p
|
| 2734 |
+
and
|
| 2735 |
+
recall
|
| 2736 |
+
( )
|
| 2737 |
+
(
|
| 2738 |
+
)
|
| 2739 |
+
*
|
| 2740 |
+
A
|
| 2741 |
+
A
|
| 2742 |
+
=
|
| 2743 |
+
−
|
| 2744 |
+
p
|
| 2745 |
+
p .
|
| 2746 |
+
Equation (33) becomes in the limit that
|
| 2747 |
+
1
|
| 2748 |
+
2
|
| 2749 |
+
→ −
|
| 2750 |
+
p
|
| 2751 |
+
p :
|
| 2752 |
+
(35)
|
| 2753 |
+
(
|
| 2754 |
+
)
|
| 2755 |
+
( )
|
| 2756 |
+
(
|
| 2757 |
+
) ( )
|
| 2758 |
+
( ) (
|
| 2759 |
+
)
|
| 2760 |
+
(
|
| 2761 |
+
)
|
| 2762 |
+
(
|
| 2763 |
+
)
|
| 2764 |
+
( )
|
| 2765 |
+
(
|
| 2766 |
+
)
|
| 2767 |
+
1
|
| 2768 |
+
2
|
| 2769 |
+
2
|
| 2770 |
+
2
|
| 2771 |
+
2
|
| 2772 |
+
2
|
| 2773 |
+
2
|
| 2774 |
+
,
|
| 2775 |
+
1
|
| 2776 |
+
2
|
| 2777 |
+
,
|
| 2778 |
+
8
|
| 2779 |
+
2
|
| 2780 |
+
0
|
| 2781 |
+
4
|
| 2782 |
+
0
|
| 2783 |
+
p
|
| 2784 |
+
p
|
| 2785 |
+
P
|
| 2786 |
+
D D
|
| 2787 |
+
D
|
| 2788 |
+
A
|
| 2789 |
+
A
|
| 2790 |
+
A
|
| 2791 |
+
A
|
| 2792 |
+
δ
|
| 2793 |
+
δ
|
| 2794 |
+
∝
|
| 2795 |
+
−
|
| 2796 |
+
−
|
| 2797 |
+
−
|
| 2798 |
+
−
|
| 2799 |
+
+
|
| 2800 |
+
p
|
| 2801 |
+
p
|
| 2802 |
+
p
|
| 2803 |
+
p
|
| 2804 |
+
p
|
| 2805 |
+
p
|
| 2806 |
+
p
|
| 2807 |
+
|
| 2808 |
+
When finding the maximum, it is the highest order delta functions that matter. Hence,
|
| 2809 |
+
only the last term needs to be considered (the second term cannot contribute a second
|
| 2810 |
+
order delta function because the piece of that term in parenthesis goes to zero) so we
|
| 2811 |
+
have, recalling the exponential term:
|
| 2812 |
+
|
| 2813 |
+
(
|
| 2814 |
+
)
|
| 2815 |
+
(
|
| 2816 |
+
)
|
| 2817 |
+
(
|
| 2818 |
+
)
|
| 2819 |
+
( )
|
| 2820 |
+
3
|
| 2821 |
+
1
|
| 2822 |
+
2
|
| 2823 |
+
2
|
| 2824 |
+
2
|
| 2825 |
+
,
|
| 2826 |
+
1
|
| 2827 |
+
2
|
| 2828 |
+
1
|
| 2829 |
+
2
|
| 2830 |
+
,
|
| 2831 |
+
4
|
| 2832 |
+
D
|
| 2833 |
+
d p
|
| 2834 |
+
p
|
| 2835 |
+
p
|
| 2836 |
+
P
|
| 2837 |
+
D D
|
| 2838 |
+
e
|
| 2839 |
+
δ
|
| 2840 |
+
−∫
|
| 2841 |
+
∝
|
| 2842 |
+
+
|
| 2843 |
+
p
|
| 2844 |
+
p
|
| 2845 |
+
p
|
| 2846 |
+
p
|
| 2847 |
+
p
|
| 2848 |
+
(
|
| 2849 |
+
1
|
| 2850 |
+
2
|
| 2851 |
+
≡
|
| 2852 |
+
= −
|
| 2853 |
+
p
|
| 2854 |
+
p
|
| 2855 |
+
p )
|
| 2856 |
+
Finding the extremum, we get:
|
| 2857 |
+
(
|
| 2858 |
+
)
|
| 2859 |
+
(
|
| 2860 |
+
)
|
| 2861 |
+
( )
|
| 2862 |
+
(
|
| 2863 |
+
)
|
| 2864 |
+
(
|
| 2865 |
+
)
|
| 2866 |
+
( )
|
| 2867 |
+
( )
|
| 2868 |
+
3
|
| 2869 |
+
3
|
| 2870 |
+
1
|
| 2871 |
+
2
|
| 2872 |
+
2
|
| 2873 |
+
2
|
| 2874 |
+
,
|
| 2875 |
+
1
|
| 2876 |
+
2
|
| 2877 |
+
1
|
| 2878 |
+
2
|
| 2879 |
+
0
|
| 2880 |
+
D
|
| 2881 |
+
d p
|
| 2882 |
+
D
|
| 2883 |
+
d p
|
| 2884 |
+
p
|
| 2885 |
+
p
|
| 2886 |
+
i
|
| 2887 |
+
i
|
| 2888 |
+
P
|
| 2889 |
+
e
|
| 2890 |
+
D
|
| 2891 |
+
e
|
| 2892 |
+
D
|
| 2893 |
+
D
|
| 2894 |
+
δ
|
| 2895 |
+
δ
|
| 2896 |
+
δ
|
| 2897 |
+
δ
|
| 2898 |
+
δ
|
| 2899 |
+
δ
|
| 2900 |
+
−
|
| 2901 |
+
−
|
| 2902 |
+
∫
|
| 2903 |
+
∫
|
| 2904 |
+
∝
|
| 2905 |
+
+
|
| 2906 |
+
= −
|
| 2907 |
+
+
|
| 2908 |
+
=
|
| 2909 |
+
p
|
| 2910 |
+
p
|
| 2911 |
+
p
|
| 2912 |
+
p
|
| 2913 |
+
p
|
| 2914 |
+
p
|
| 2915 |
+
p
|
| 2916 |
+
p
|
| 2917 |
+
p
|
| 2918 |
+
p
|
| 2919 |
+
|
| 2920 |
+
So,
|
| 2921 |
+
( )
|
| 2922 |
+
0
|
| 2923 |
+
D
|
| 2924 |
+
=
|
| 2925 |
+
p
|
| 2926 |
+
, which means that there is no average energy in this mode in the most
|
| 2927 |
+
likely A amplitude distribution.
|
| 2928 |
+
Conclusion
|
| 2929 |
+
|
| 2930 |
+
We have here given the structure of the photon vector potential distribution and
|
| 2931 |
+
theoretically derived, for the first time, its key feature, thus enlightening long held,
|
| 2932 |
+
though often confused, intuitions about photons.
|
| 2933 |
+
|
| 2934 |
+
Like all references to quantum mechanical states, the term photon refers to a
|
| 2935 |
+
system statistically, not individually; quantum mechanics only predicts probable
|
| 2936 |
+
outcomes, so needs many experiments on different systems (experiments on an
|
| 2937 |
+
“ensemble” of systems) in the same state (or approximately the same state) to verify the
|
| 2938 |
+
prediction. This paper proves that a photonic state is a state which has a stochastic vector
|
| 2939 |
+
potential (A) filling space whose most likely amplitude (magnitude) structure (across the
|
| 2940 |
+
ensemble of systems) has a sinewave component of frequency
|
| 2941 |
+
/ h
|
| 2942 |
+
p
|
| 2943 |
+
for each photon of
|
| 2944 |
+
momentum p in the system. Getting this insight into the free field states, being
|
| 2945 |
+
fundamental, can build intuition into other more complicated (e.g., interactional) QFT
|
| 2946 |
+
problems.
|
| 2947 |
+
|
| 2948 |
+
Recognizing the stochastic character of the QFT states can lead one to introduce
|
| 2949 |
+
Parseval’s theorem (and other statistical theorems) which along with the Schrödinger
|
| 2950 |
+
formalism are intuitive tools and are required to get these results. The QFT analog of the
|
| 2951 |
+
Schrödinger equation allows one to carry all the intuition one gained in ordinary quantum
|
| 2952 |
+
mechanics about waves and particles over to QFT, including into Yang Mill’s theory. It
|
| 2953 |
+
has been used in attempts to use QFT in general relativity in a 3+1 space time setting,
|
| 2954 |
+
which also points to its draw back that it is not explicitly relativistically invariant.21 It is
|
| 2955 |
+
|
| 2956 |
+
21 D.V. Long, G.M. Shore, The Schrödinger Wave Functional and Vacuum States in Curved Spacetime,
|
| 2957 |
+
Nucl. Phys. B 530, 247-278 (1998) D.V. Long, G.M. Shore, The Schrodinger Wave Functional and
|
| 2958 |
+
Vacuum States in Curved Spacetime II: Boundaries and Foliations, Nucl. Phys. B 530, 279-303 (1998).
|
| 2959 |
+
P.R. Holland, The De Broglie-Bohm Theory of Motion and Quantum Field Theory, Phys. Rept. 224 No. 3,
|
| 2960 |
+
|
| 2961 |
+
11
|
| 2962 |
+
|
| 2963 |
+
also required and used in interesting ways in De Broglie-Bohm (dBB) formalism of
|
| 2964 |
+
QFT.22 Though this work fills a lacunae and is foundational (further demonstrating the
|
| 2965 |
+
nature of the fundamental entity “photon”), it requires the relatively infrequently used
|
| 2966 |
+
QFT Schrödinger formalism and this seems to be part of why it has been overlooked till
|
| 2967 |
+
now. Hopefully, this filling of the lacunae will help spur the use of the Schrödinger
|
| 2968 |
+
formalism and thereby make available the attending insights offered by its distinct
|
| 2969 |
+
perspective on QFT.23,24
|
| 2970 |
+
|
| 2971 |
+
|
| 2972 |
+
Appendix A
|
| 2973 |
+
Calculation of the wave-functionals for 2, 3 and 4 photon systems.
|
| 2974 |
+
(36)
|
| 2975 |
+
|
| 2976 |
+
( )
|
| 2977 |
+
(
|
| 2978 |
+
)
|
| 2979 |
+
(
|
| 2980 |
+
)
|
| 2981 |
+
†
|
| 2982 |
+
0
|
| 2983 |
+
n
|
| 2984 |
+
i
|
| 2985 |
+
i
|
| 2986 |
+
i
|
| 2987 |
+
i
|
| 2988 |
+
n
|
| 2989 |
+
A
|
| 2990 |
+
A n
|
| 2991 |
+
A n
|
| 2992 |
+
A
|
| 2993 |
+
a
|
| 2994 |
+
Ψ
|
| 2995 |
+
=
|
| 2996 |
+
=
|
| 2997 |
+
=
|
| 2998 |
+
p
|
| 2999 |
+
p
|
| 3000 |
+
p
|
| 3001 |
+
x
|
| 3002 |
+
p
|
| 3003 |
+
,
|
| 3004 |
+
Substituting (7) and generalizing from (8):
|
| 3005 |
+
(37)
|
| 3006 |
+
( )
|
| 3007 |
+
(
|
| 3008 |
+
)
|
| 3009 |
+
(
|
| 3010 |
+
)
|
| 3011 |
+
(
|
| 3012 |
+
)
|
| 3013 |
+
( )
|
| 3014 |
+
( )
|
| 3015 |
+
3
|
| 3016 |
+
3 /2
|
| 3017 |
+
/2
|
| 3018 |
+
1
|
| 3019 |
+
1
|
| 3020 |
+
ˆ
|
| 3021 |
+
0
|
| 3022 |
+
2
|
| 3023 |
+
2
|
| 3024 |
+
n
|
| 3025 |
+
i
|
| 3026 |
+
i
|
| 3027 |
+
i
|
| 3028 |
+
i
|
| 3029 |
+
n
|
| 3030 |
+
n
|
| 3031 |
+
i
|
| 3032 |
+
A
|
| 3033 |
+
A
|
| 3034 |
+
e
|
| 3035 |
+
E A
|
| 3036 |
+
d x
|
| 3037 |
+
A
|
| 3038 |
+
E
|
| 3039 |
+
δ
|
| 3040 |
+
δ
|
| 3041 |
+
π
|
| 3042 |
+
⋅
|
| 3043 |
+
⎛
|
| 3044 |
+
⎞
|
| 3045 |
+
⎛
|
| 3046 |
+
⎞
|
| 3047 |
+
Ψ
|
| 3048 |
+
=
|
| 3049 |
+
−
|
| 3050 |
+
⎜
|
| 3051 |
+
⎟
|
| 3052 |
+
⎜
|
| 3053 |
+
⎟
|
| 3054 |
+
⎜
|
| 3055 |
+
⎟
|
| 3056 |
+
⎝
|
| 3057 |
+
⎠
|
| 3058 |
+
⎝
|
| 3059 |
+
⎠
|
| 3060 |
+
∫
|
| 3061 |
+
p x
|
| 3062 |
+
np
|
| 3063 |
+
p
|
| 3064 |
+
p
|
| 3065 |
+
x
|
| 3066 |
+
x
|
| 3067 |
+
x
|
| 3068 |
+
|
| 3069 |
+
|
| 3070 |
+
Note: we will need to use:
|
| 3071 |
+
( )
|
| 3072 |
+
( )
|
| 3073 |
+
i
|
| 3074 |
+
A
|
| 3075 |
+
e
|
| 3076 |
+
A
|
| 3077 |
+
δ
|
| 3078 |
+
δ
|
| 3079 |
+
−
|
| 3080 |
+
⋅
|
| 3081 |
+
=
|
| 3082 |
+
�
|
| 3083 |
+
p x
|
| 3084 |
+
p
|
| 3085 |
+
x
|
| 3086 |
+
(and perhaps
|
| 3087 |
+
( )
|
| 3088 |
+
( )
|
| 3089 |
+
i
|
| 3090 |
+
A
|
| 3091 |
+
e
|
| 3092 |
+
A
|
| 3093 |
+
δ
|
| 3094 |
+
δ
|
| 3095 |
+
⋅
|
| 3096 |
+
=
|
| 3097 |
+
�
|
| 3098 |
+
p x
|
| 3099 |
+
x
|
| 3100 |
+
p
|
| 3101 |
+
)
|
| 3102 |
+
Dropping multiplicative factors to reduce space and focus on form of the equations, we
|
| 3103 |
+
can write the generic equation that we will use below:
|
| 3104 |
+
(38)
|
| 3105 |
+
( )
|
| 3106 |
+
(
|
| 3107 |
+
)
|
| 3108 |
+
(
|
| 3109 |
+
)
|
| 3110 |
+
( )
|
| 3111 |
+
(
|
| 3112 |
+
)
|
| 3113 |
+
( )
|
| 3114 |
+
(
|
| 3115 |
+
)
|
| 3116 |
+
1
|
| 3117 |
+
i
|
| 3118 |
+
i
|
| 3119 |
+
i
|
| 3120 |
+
n
|
| 3121 |
+
p
|
| 3122 |
+
i
|
| 3123 |
+
A
|
| 3124 |
+
A
|
| 3125 |
+
A
|
| 3126 |
+
A
|
| 3127 |
+
δ
|
| 3128 |
+
δ
|
| 3129 |
+
−
|
| 3130 |
+
⎛
|
| 3131 |
+
⎞
|
| 3132 |
+
Ψ
|
| 3133 |
+
==
|
| 3134 |
+
−
|
| 3135 |
+
−
|
| 3136 |
+
Ψ
|
| 3137 |
+
⎜
|
| 3138 |
+
⎟
|
| 3139 |
+
⎝
|
| 3140 |
+
⎠
|
| 3141 |
+
�
|
| 3142 |
+
�
|
| 3143 |
+
np
|
| 3144 |
+
x
|
| 3145 |
+
p
|
| 3146 |
+
p
|
| 3147 |
+
x
|
| 3148 |
+
p
|
| 3149 |
+
|
| 3150 |
+
Using this and recalling
|
| 3151 |
+
( )
|
| 3152 |
+
(
|
| 3153 |
+
)
|
| 3154 |
+
(
|
| 3155 |
+
)
|
| 3156 |
+
( )
|
| 3157 |
+
3
|
| 3158 |
+
1
|
| 3159 |
+
2
|
| 3160 |
+
2
|
| 3161 |
+
i
|
| 3162 |
+
i
|
| 3163 |
+
d
|
| 3164 |
+
A
|
| 3165 |
+
p
|
| 3166 |
+
i
|
| 3167 |
+
e
|
| 3168 |
+
A
|
| 3169 |
+
A
|
| 3170 |
+
2
|
| 3171 |
+
−
|
| 3172 |
+
Ψ
|
| 3173 |
+
=
|
| 3174 |
+
∫
|
| 3175 |
+
−
|
| 3176 |
+
�
|
| 3177 |
+
p
|
| 3178 |
+
p
|
| 3179 |
+
p
|
| 3180 |
+
x
|
| 3181 |
+
p
|
| 3182 |
+
p
|
| 3183 |
+
, we now calculate the 2,
|
| 3184 |
+
3 and 4 photon wavefunctionals.
|
| 3185 |
+
|
| 3186 |
+
n=2 case :
|
| 3187 |
+
|
| 3188 |
+
95-150 (1993), N. Pinto-Neto, J. C. Fabris, Quantum Cosmology from the De Broglie-Bohm Perspective,
|
| 3189 |
+
Class. Quantum Grav. 30 No. 143001, 57 (2013).
|
| 3190 |
+
22 P.R. Holland, The De Broglie-Bohm Theory of Motion and Quantum Field Theory, Phys. Rept. 224 No.
|
| 3191 |
+
3, 95-150 (1993), N. Pinto-Neto, J. C. Fabris, Quantum Cosmology from the De Broglie-Bohm
|
| 3192 |
+
Perspective, Class. Quantum Grav. 30 No. 143001, 57 (2013).others P. Roser, A. Valentini, Classical and
|
| 3193 |
+
Quantum Cosmology with York Time, Class. Quantum Grav. 31 No. 245001 (2014). See other papers by
|
| 3194 |
+
P.R. Holland which use Schrödinger approach relative to the dBB interpretation of quantum mechanics,
|
| 3195 |
+
and A. Valentini’s papers on dBB applied to quantum cosmology.
|
| 3196 |
+
23 C. Kiefer, Functional Schrodinger Equation for Scalar QED, Phys. Rev. D 45 No. 6, 2044-2056, (1992)
|
| 3197 |
+
24 Also, the use of functionals cross fertilizes with their use in the path integral formulation as well as,
|
| 3198 |
+
through the functional Schrödinger equation, evokes the functional domain analog of the path from the
|
| 3199 |
+
Schrödinger equation to path integrals.
|
| 3200 |
+
|
| 3201 |
+
12
|
| 3202 |
+
|
| 3203 |
+
(39)
|
| 3204 |
+
( )
|
| 3205 |
+
(
|
| 3206 |
+
)
|
| 3207 |
+
(
|
| 3208 |
+
)
|
| 3209 |
+
( )
|
| 3210 |
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(
|
| 3211 |
+
)
|
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+
( )
|
| 3213 |
+
( )
|
| 3214 |
+
(
|
| 3215 |
+
)
|
| 3216 |
+
0
|
| 3217 |
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i
|
| 3218 |
+
i
|
| 3219 |
+
i
|
| 3220 |
+
i
|
| 3221 |
+
i
|
| 3222 |
+
i
|
| 3223 |
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|
| 3224 |
+
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|
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A
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+
A
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| 3227 |
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A
|
| 3228 |
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|
| 3229 |
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| 3230 |
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δ
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| 3231 |
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δ
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| 3232 |
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| 3235 |
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| 3237 |
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p
|
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+
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|
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+
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i
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|
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|
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|
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|
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|
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|
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|
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|
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|
| 3454 |
+
n=3 case:
|
| 3455 |
+
(40)
|
| 3456 |
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|
| 3457 |
+
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|
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|
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+
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|
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|
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3
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|
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|
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|
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|
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|
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|
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|
| 3660 |
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|
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|
| 3664 |
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|
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|
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|
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|
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|
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+
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|
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|
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+
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|
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|
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+
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|
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|
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|
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+
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|
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|
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|
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+
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|
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3
|
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1
|
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3
|
| 3683 |
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2
|
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2
|
| 3685 |
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|
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2
|
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3
|
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2
|
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|
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p
|
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|
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i
|
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+
i
|
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+
d
|
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e
|
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A
|
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+
A
|
| 3698 |
+
A
|
| 3699 |
+
δ
|
| 3700 |
+
2
|
| 3701 |
+
−
|
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+
Ψ
|
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+
=
|
| 3704 |
+
−
|
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+
−
|
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−
|
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∫
|
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|
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|
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p
|
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p
|
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3p
|
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x
|
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+
p
|
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+
p
|
| 3716 |
+
p
|
| 3717 |
+
p
|
| 3718 |
+
p
|
| 3719 |
+
|
| 3720 |
+
|
| 3721 |
+
n=4 case:
|
| 3722 |
+
|
| 3723 |
+
(41)
|
| 3724 |
+
( )
|
| 3725 |
+
(
|
| 3726 |
+
)
|
| 3727 |
+
(
|
| 3728 |
+
)
|
| 3729 |
+
( )
|
| 3730 |
+
( )
|
| 3731 |
+
(
|
| 3732 |
+
)
|
| 3733 |
+
i
|
| 3734 |
+
i
|
| 3735 |
+
i
|
| 3736 |
+
i
|
| 3737 |
+
A
|
| 3738 |
+
A
|
| 3739 |
+
A
|
| 3740 |
+
A
|
| 3741 |
+
δ
|
| 3742 |
+
δ
|
| 3743 |
+
⎛
|
| 3744 |
+
⎞
|
| 3745 |
+
Ψ
|
| 3746 |
+
=
|
| 3747 |
+
−
|
| 3748 |
+
−
|
| 3749 |
+
Ψ
|
| 3750 |
+
⎜
|
| 3751 |
+
⎟
|
| 3752 |
+
⎝
|
| 3753 |
+
⎠
|
| 3754 |
+
�
|
| 3755 |
+
�
|
| 3756 |
+
4 p
|
| 3757 |
+
3 p
|
| 3758 |
+
x
|
| 3759 |
+
p
|
| 3760 |
+
p
|
| 3761 |
+
x
|
| 3762 |
+
p
|
| 3763 |
+
|
| 3764 |
+
|
| 3765 |
+
|
| 3766 |
+
13
|
| 3767 |
+
|
| 3768 |
+
|
| 3769 |
+
|
| 3770 |
+
(
|
| 3771 |
+
)
|
| 3772 |
+
(
|
| 3773 |
+
)
|
| 3774 |
+
(
|
| 3775 |
+
)
|
| 3776 |
+
(
|
| 3777 |
+
)
|
| 3778 |
+
(
|
| 3779 |
+
) (
|
| 3780 |
+
)
|
| 3781 |
+
(
|
| 3782 |
+
)
|
| 3783 |
+
( )
|
| 3784 |
+
(
|
| 3785 |
+
)
|
| 3786 |
+
(
|
| 3787 |
+
)
|
| 3788 |
+
(
|
| 3789 |
+
)
|
| 3790 |
+
(
|
| 3791 |
+
) (
|
| 3792 |
+
)
|
| 3793 |
+
(
|
| 3794 |
+
)
|
| 3795 |
+
( )
|
| 3796 |
+
( )
|
| 3797 |
+
3
|
| 3798 |
+
3
|
| 3799 |
+
3
|
| 3800 |
+
2
|
| 3801 |
+
3
|
| 3802 |
+
1
|
| 3803 |
+
2
|
| 3804 |
+
1
|
| 3805 |
+
2
|
| 3806 |
+
2
|
| 3807 |
+
3
|
| 3808 |
+
2
|
| 3809 |
+
4
|
| 3810 |
+
2
|
| 3811 |
+
3
|
| 3812 |
+
2
|
| 3813 |
+
i
|
| 3814 |
+
i
|
| 3815 |
+
d
|
| 3816 |
+
A
|
| 3817 |
+
p
|
| 3818 |
+
i
|
| 3819 |
+
i
|
| 3820 |
+
i
|
| 3821 |
+
A
|
| 3822 |
+
i
|
| 3823 |
+
i
|
| 3824 |
+
d p
|
| 3825 |
+
i
|
| 3826 |
+
e
|
| 3827 |
+
e
|
| 3828 |
+
A
|
| 3829 |
+
A
|
| 3830 |
+
A
|
| 3831 |
+
A
|
| 3832 |
+
A
|
| 3833 |
+
A
|
| 3834 |
+
δ
|
| 3835 |
+
δ
|
| 3836 |
+
δ
|
| 3837 |
+
δ
|
| 3838 |
+
2
|
| 3839 |
+
2
|
| 3840 |
+
−
|
| 3841 |
+
−
|
| 3842 |
+
⎛
|
| 3843 |
+
⎞
|
| 3844 |
+
−
|
| 3845 |
+
−
|
| 3846 |
+
−
|
| 3847 |
+
−
|
| 3848 |
+
⎜
|
| 3849 |
+
⎟
|
| 3850 |
+
⎜
|
| 3851 |
+
⎟
|
| 3852 |
+
⎜
|
| 3853 |
+
⎟
|
| 3854 |
+
⎛
|
| 3855 |
+
⎞
|
| 3856 |
+
=
|
| 3857 |
+
−
|
| 3858 |
+
−
|
| 3859 |
+
−
|
| 3860 |
+
⎜
|
| 3861 |
+
⎟
|
| 3862 |
+
⎜
|
| 3863 |
+
⎟
|
| 3864 |
+
⎝
|
| 3865 |
+
⎠
|
| 3866 |
+
⎜
|
| 3867 |
+
∫
|
| 3868 |
+
∫
|
| 3869 |
+
⎟
|
| 3870 |
+
−
|
| 3871 |
+
⎜
|
| 3872 |
+
⎟
|
| 3873 |
+
⎝
|
| 3874 |
+
⎠
|
| 3875 |
+
�
|
| 3876 |
+
�
|
| 3877 |
+
�
|
| 3878 |
+
�
|
| 3879 |
+
�
|
| 3880 |
+
�
|
| 3881 |
+
p
|
| 3882 |
+
p
|
| 3883 |
+
p
|
| 3884 |
+
p
|
| 3885 |
+
p
|
| 3886 |
+
p
|
| 3887 |
+
p
|
| 3888 |
+
p
|
| 3889 |
+
p
|
| 3890 |
+
p
|
| 3891 |
+
p
|
| 3892 |
+
p
|
| 3893 |
+
p
|
| 3894 |
+
p
|
| 3895 |
+
p
|
| 3896 |
+
p
|
| 3897 |
+
|
| 3898 |
+
|
| 3899 |
+
(
|
| 3900 |
+
)
|
| 3901 |
+
(
|
| 3902 |
+
)
|
| 3903 |
+
(
|
| 3904 |
+
)
|
| 3905 |
+
(
|
| 3906 |
+
)
|
| 3907 |
+
(
|
| 3908 |
+
)
|
| 3909 |
+
(
|
| 3910 |
+
)
|
| 3911 |
+
(
|
| 3912 |
+
)
|
| 3913 |
+
(
|
| 3914 |
+
)
|
| 3915 |
+
(
|
| 3916 |
+
)
|
| 3917 |
+
(
|
| 3918 |
+
)
|
| 3919 |
+
(
|
| 3920 |
+
)
|
| 3921 |
+
(
|
| 3922 |
+
)
|
| 3923 |
+
(
|
| 3924 |
+
)
|
| 3925 |
+
(
|
| 3926 |
+
)
|
| 3927 |
+
(
|
| 3928 |
+
) (
|
| 3929 |
+
)
|
| 3930 |
+
(
|
| 3931 |
+
)
|
| 3932 |
+
(
|
| 3933 |
+
)
|
| 3934 |
+
( )
|
| 3935 |
+
3
|
| 3936 |
+
4
|
| 3937 |
+
2
|
| 3938 |
+
2
|
| 3939 |
+
2
|
| 3940 |
+
2
|
| 3941 |
+
1
|
| 3942 |
+
2
|
| 3943 |
+
2
|
| 3944 |
+
3
|
| 3945 |
+
2
|
| 3946 |
+
3
|
| 3947 |
+
2
|
| 3948 |
+
4
|
| 3949 |
+
6
|
| 3950 |
+
2
|
| 3951 |
+
3
|
| 3952 |
+
2
|
| 3953 |
+
2
|
| 3954 |
+
3
|
| 3955 |
+
2
|
| 3956 |
+
i
|
| 3957 |
+
i
|
| 3958 |
+
i
|
| 3959 |
+
A
|
| 3960 |
+
p
|
| 3961 |
+
i
|
| 3962 |
+
i
|
| 3963 |
+
i
|
| 3964 |
+
d
|
| 3965 |
+
i
|
| 3966 |
+
A
|
| 3967 |
+
A
|
| 3968 |
+
A
|
| 3969 |
+
A
|
| 3970 |
+
A
|
| 3971 |
+
A
|
| 3972 |
+
e
|
| 3973 |
+
δ
|
| 3974 |
+
δ
|
| 3975 |
+
δ
|
| 3976 |
+
δ
|
| 3977 |
+
2
|
| 3978 |
+
−
|
| 3979 |
+
⎛
|
| 3980 |
+
⎞
|
| 3981 |
+
−
|
| 3982 |
+
−
|
| 3983 |
+
⎜
|
| 3984 |
+
⎟
|
| 3985 |
+
=
|
| 3986 |
+
⎜
|
| 3987 |
+
⎟
|
| 3988 |
+
−
|
| 3989 |
+
−
|
| 3990 |
+
−
|
| 3991 |
+
−
|
| 3992 |
+
−
|
| 3993 |
+
−
|
| 3994 |
+
−
|
| 3995 |
+
−
|
| 3996 |
+
⎜
|
| 3997 |
+
⎟
|
| 3998 |
+
⎝
|
| 3999 |
+
⎠
|
| 4000 |
+
∫
|
| 4001 |
+
�
|
| 4002 |
+
�
|
| 4003 |
+
�
|
| 4004 |
+
�
|
| 4005 |
+
�
|
| 4006 |
+
�
|
| 4007 |
+
p
|
| 4008 |
+
p
|
| 4009 |
+
p
|
| 4010 |
+
p
|
| 4011 |
+
p
|
| 4012 |
+
-p
|
| 4013 |
+
p
|
| 4014 |
+
p
|
| 4015 |
+
p
|
| 4016 |
+
p
|
| 4017 |
+
p
|
| 4018 |
+
p
|
| 4019 |
+
p
|
| 4020 |
+
p
|
| 4021 |
+
p
|
| 4022 |
+
p
|
| 4023 |
+
p
|
| 4024 |
+
p
|
| 4025 |
+
|
| 4026 |
+
So,
|
| 4027 |
+
( )
|
| 4028 |
+
(
|
| 4029 |
+
)
|
| 4030 |
+
(
|
| 4031 |
+
)
|
| 4032 |
+
(
|
| 4033 |
+
)
|
| 4034 |
+
(
|
| 4035 |
+
)
|
| 4036 |
+
(
|
| 4037 |
+
)
|
| 4038 |
+
(
|
| 4039 |
+
)
|
| 4040 |
+
(
|
| 4041 |
+
)
|
| 4042 |
+
(
|
| 4043 |
+
)
|
| 4044 |
+
(
|
| 4045 |
+
)
|
| 4046 |
+
( )
|
| 4047 |
+
3
|
| 4048 |
+
4
|
| 4049 |
+
2
|
| 4050 |
+
2
|
| 4051 |
+
2
|
| 4052 |
+
2
|
| 4053 |
+
1
|
| 4054 |
+
2
|
| 4055 |
+
4
|
| 4056 |
+
4
|
| 4057 |
+
12
|
| 4058 |
+
2
|
| 4059 |
+
3
|
| 4060 |
+
2
|
| 4061 |
+
iA
|
| 4062 |
+
p
|
| 4063 |
+
i
|
| 4064 |
+
i
|
| 4065 |
+
i
|
| 4066 |
+
d
|
| 4067 |
+
A
|
| 4068 |
+
e
|
| 4069 |
+
A
|
| 4070 |
+
A
|
| 4071 |
+
δ
|
| 4072 |
+
δ
|
| 4073 |
+
2
|
| 4074 |
+
−
|
| 4075 |
+
Ψ
|
| 4076 |
+
=
|
| 4077 |
+
−
|
| 4078 |
+
−
|
| 4079 |
+
+
|
| 4080 |
+
∫
|
| 4081 |
+
�
|
| 4082 |
+
�
|
| 4083 |
+
p
|
| 4084 |
+
p
|
| 4085 |
+
4p
|
| 4086 |
+
x
|
| 4087 |
+
p
|
| 4088 |
+
p
|
| 4089 |
+
p
|
| 4090 |
+
p
|
| 4091 |
+
-p
|
| 4092 |
+
p
|
| 4093 |
+
p
|
| 4094 |
+
|
| 4095 |
+
Recalling that finally we take
|
| 4096 |
+
0
|
| 4097 |
+
≠
|
| 4098 |
+
p
|
| 4099 |
+
, we first drop the squared deltas:
|
| 4100 |
+
( )
|
| 4101 |
+
(
|
| 4102 |
+
)
|
| 4103 |
+
(
|
| 4104 |
+
)
|
| 4105 |
+
(
|
| 4106 |
+
)
|
| 4107 |
+
(
|
| 4108 |
+
)
|
| 4109 |
+
(
|
| 4110 |
+
)
|
| 4111 |
+
(
|
| 4112 |
+
)
|
| 4113 |
+
(
|
| 4114 |
+
)
|
| 4115 |
+
( )
|
| 4116 |
+
3
|
| 4117 |
+
3
|
| 4118 |
+
1
|
| 4119 |
+
4
|
| 4120 |
+
2
|
| 4121 |
+
2
|
| 4122 |
+
16
|
| 4123 |
+
3
|
| 4124 |
+
2
|
| 4125 |
+
iA
|
| 4126 |
+
i
|
| 4127 |
+
d p
|
| 4128 |
+
i
|
| 4129 |
+
i
|
| 4130 |
+
e
|
| 4131 |
+
A
|
| 4132 |
+
A
|
| 4133 |
+
A
|
| 4134 |
+
δ
|
| 4135 |
+
2
|
| 4136 |
+
−
|
| 4137 |
+
Ψ
|
| 4138 |
+
==
|
| 4139 |
+
−
|
| 4140 |
+
−
|
| 4141 |
+
−
|
| 4142 |
+
∫
|
| 4143 |
+
�
|
| 4144 |
+
�
|
| 4145 |
+
p
|
| 4146 |
+
p
|
| 4147 |
+
4p
|
| 4148 |
+
x
|
| 4149 |
+
p
|
| 4150 |
+
p
|
| 4151 |
+
p
|
| 4152 |
+
p
|
| 4153 |
+
p
|
| 4154 |
+
|
| 4155 |
+
Ignoring the delta function completely gives:
|
| 4156 |
+
( )
|
| 4157 |
+
(
|
| 4158 |
+
)
|
| 4159 |
+
(
|
| 4160 |
+
)
|
| 4161 |
+
(
|
| 4162 |
+
)
|
| 4163 |
+
( )
|
| 4164 |
+
3
|
| 4165 |
+
4
|
| 4166 |
+
4
|
| 4167 |
+
1
|
| 4168 |
+
2
|
| 4169 |
+
16
|
| 4170 |
+
iA
|
| 4171 |
+
p
|
| 4172 |
+
i
|
| 4173 |
+
i
|
| 4174 |
+
d
|
| 4175 |
+
e
|
| 4176 |
+
A
|
| 4177 |
+
A
|
| 4178 |
+
2
|
| 4179 |
+
−
|
| 4180 |
+
Ψ
|
| 4181 |
+
=
|
| 4182 |
+
−
|
| 4183 |
+
∫
|
| 4184 |
+
�
|
| 4185 |
+
p
|
| 4186 |
+
p
|
| 4187 |
+
4p
|
| 4188 |
+
x
|
| 4189 |
+
p
|
| 4190 |
+
p
|
| 4191 |
+
|
| 4192 |
+
|
F9FJT4oBgHgl3EQfDixl/content/tmp_files/load_file.txt
ADDED
|
The diff for this file is too large to render.
See raw diff
|
|
|
GNAzT4oBgHgl3EQfUfzc/content/tmp_files/2301.01269v1.pdf.txt
ADDED
|
@@ -0,0 +1,1110 @@
|
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|
|
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|
| 1 |
+
Average Is Not Enough: Caveats of Multilingual Evaluation
|
| 2 |
+
Matúš Pikuliak and Marián Šimko
|
| 3 |
+
Kempelen Institute of Intelligent Technologies
|
| 4 |
+
firstname.surname@kinit.sk
|
| 5 |
+
Abstract
|
| 6 |
+
This position paper discusses the problem of
|
| 7 |
+
multilingual evaluation. Using simple statis-
|
| 8 |
+
tics, such as average language performance,
|
| 9 |
+
might inject linguistic biases in favor of domi-
|
| 10 |
+
nant language families into evaluation method-
|
| 11 |
+
ology. We argue that a qualitative analysis in-
|
| 12 |
+
formed by comparative linguistics is needed
|
| 13 |
+
for multilingual results to detect this kind of
|
| 14 |
+
bias. We show in our case study that results in
|
| 15 |
+
published works can indeed be linguistically
|
| 16 |
+
biased and we demonstrate that visualization
|
| 17 |
+
based on URIEL typological database can de-
|
| 18 |
+
tect it.
|
| 19 |
+
1
|
| 20 |
+
Introduction
|
| 21 |
+
The linguistic diversity of NLP research is grow-
|
| 22 |
+
ing (Joshi et al., 2020; Pikuliak et al., 2021) thanks
|
| 23 |
+
to improvements of various multilingual technolo-
|
| 24 |
+
gies, such as machine translation (Arivazhagan
|
| 25 |
+
et al., 2019), multilingual language models (Devlin
|
| 26 |
+
et al., 2019; Conneau and Lample, 2019), cross-
|
| 27 |
+
lingual transfer learning (Pikuliak et al., 2021) or
|
| 28 |
+
language independent representations (Ruder et al.,
|
| 29 |
+
2019). It is now possible to create well-performing
|
| 30 |
+
multilingual methods for many tasks. When deal-
|
| 31 |
+
ing with multilingual methods, we need to be able
|
| 32 |
+
to evaluate how good they really are, i.e. how effec-
|
| 33 |
+
tive they are on a wide variety of typologically di-
|
| 34 |
+
verse languages. Consider the two methods shown
|
| 35 |
+
in Figure 1 (a). Without looking at the particular
|
| 36 |
+
languages, Method A seems better. It has better re-
|
| 37 |
+
sults for the majority of languages and its average
|
| 38 |
+
performance is better as well. However, the trio
|
| 39 |
+
of languages, where Method A is better, are in fact
|
| 40 |
+
all very similar Iberian languages, while the fourth
|
| 41 |
+
language is Indo-Iranian. Is the Method A actually
|
| 42 |
+
better, or is it better only for Iberian? Simple av-
|
| 43 |
+
erage is often used in practice without considering
|
| 44 |
+
the linguistic diversity of the underlying selection
|
| 45 |
+
of languages, despite the fact that many corpora
|
| 46 |
+
and datasets are biased in favor of historically dom-
|
| 47 |
+
inant languages and language families.
|
| 48 |
+
Additionally, as the number of languages in-
|
| 49 |
+
creases, it is harder and harder to notice phenomena
|
| 50 |
+
such as this. Consider the comparison of two sets
|
| 51 |
+
of results in Table 1. With 41 languages it is cog-
|
| 52 |
+
nitively hard to discover various relations between
|
| 53 |
+
the languages and their results, even if one has the
|
| 54 |
+
necessary linguistic knowledge.
|
| 55 |
+
In this position paper, we argue that it is not
|
| 56 |
+
the best practice to compare multilingual methods
|
| 57 |
+
only with simple statistics, such as average. Com-
|
| 58 |
+
monly used simple evaluation protocols might bias
|
| 59 |
+
research in favor of dominant languages and in turn
|
| 60 |
+
hurt historically marginalized languages. Instead,
|
| 61 |
+
we propose to consider using qualitative results
|
| 62 |
+
analysis that takes linguistic typology (Ponti et al.,
|
| 63 |
+
2019) and comparative linguistics into account as
|
| 64 |
+
an additional sanity check. We believe that this
|
| 65 |
+
is an often overlooked tool in our research toolkit
|
| 66 |
+
that should be used more to ensure that we are
|
| 67 |
+
able to properly interpret results from multilingual
|
| 68 |
+
evaluation and detect various linguistic biases and
|
| 69 |
+
problems. In addition to this discussion, which
|
| 70 |
+
we consider a contribution in itself, we also pro-
|
| 71 |
+
pose a visualization based on URIEL typological
|
| 72 |
+
database (Littell et al., 2017) as an example of such
|
| 73 |
+
qualitative analysis, and we show that it is able to
|
| 74 |
+
discover linguistic biases in published results.
|
| 75 |
+
2
|
| 76 |
+
Related Work
|
| 77 |
+
Linguistic biases in NLP.
|
| 78 |
+
Bender (2009) postu-
|
| 79 |
+
lated that research driven mainly by evaluation in
|
| 80 |
+
English will become biased in favor of this lan-
|
| 81 |
+
guage and it might not be particularly language
|
| 82 |
+
independent. Even in recent years, popular tech-
|
| 83 |
+
niques such as word2vec or Byte Pair Encoding
|
| 84 |
+
were shown to have worse performance on morpho-
|
| 85 |
+
logically rich languages (Bojanowski et al., 2017;
|
| 86 |
+
Park et al., 2020). Similarly, cross-lingual word
|
| 87 |
+
embeddings are usually constructed with English
|
| 88 |
+
arXiv:2301.01269v1 [cs.CL] 3 Jan 2023
|
| 89 |
+
|
| 90 |
+
Spanish
|
| 91 |
+
Catalan
|
| 92 |
+
Portugese
|
| 93 |
+
Persian
|
| 94 |
+
Average
|
| 95 |
+
Performance
|
| 96 |
+
76.0
|
| 97 |
+
79.0
|
| 98 |
+
74.0
|
| 99 |
+
52.0
|
| 100 |
+
70.25
|
| 101 |
+
63.0
|
| 102 |
+
62.0
|
| 103 |
+
59.0
|
| 104 |
+
74.0
|
| 105 |
+
64.5
|
| 106 |
+
(a)
|
| 107 |
+
Method A
|
| 108 |
+
Method B
|
| 109 |
+
Atlantic-Congo
|
| 110 |
+
Afro-Asiatic
|
| 111 |
+
Semitic
|
| 112 |
+
Pama-Nyungan
|
| 113 |
+
Otomanguean
|
| 114 |
+
Italic
|
| 115 |
+
Slavic
|
| 116 |
+
Germanic
|
| 117 |
+
Uralic
|
| 118 |
+
Indo-Iranian
|
| 119 |
+
Dravidian
|
| 120 |
+
Turkic
|
| 121 |
+
Sino-Tibetan
|
| 122 |
+
Austroasiatic
|
| 123 |
+
Austronesian
|
| 124 |
+
(b)
|
| 125 |
+
(c)
|
| 126 |
+
Figure 1: (a) Comparison of two methods on unbalanced set of languages. (b) Visualization of URIEL languages
|
| 127 |
+
with certain language families color-coded. (c) Comparison of two methods from Rahimi et al. This uses the same
|
| 128 |
+
map of languages as b, but the view is zoomed.
|
| 129 |
+
Language
|
| 130 |
+
afr
|
| 131 |
+
arb
|
| 132 |
+
bul
|
| 133 |
+
ben
|
| 134 |
+
bos
|
| 135 |
+
cat
|
| 136 |
+
ces
|
| 137 |
+
dan
|
| 138 |
+
deu
|
| 139 |
+
ell
|
| 140 |
+
eng
|
| 141 |
+
spa
|
| 142 |
+
est
|
| 143 |
+
pes
|
| 144 |
+
fin
|
| 145 |
+
fra
|
| 146 |
+
heb
|
| 147 |
+
hin
|
| 148 |
+
hrv
|
| 149 |
+
hun
|
| 150 |
+
ind
|
| 151 |
+
Method A
|
| 152 |
+
74
|
| 153 |
+
54
|
| 154 |
+
54
|
| 155 |
+
60
|
| 156 |
+
77
|
| 157 |
+
79
|
| 158 |
+
72
|
| 159 |
+
79
|
| 160 |
+
64
|
| 161 |
+
34
|
| 162 |
+
57
|
| 163 |
+
76
|
| 164 |
+
71
|
| 165 |
+
52
|
| 166 |
+
69
|
| 167 |
+
73
|
| 168 |
+
46
|
| 169 |
+
58
|
| 170 |
+
77
|
| 171 |
+
69
|
| 172 |
+
61
|
| 173 |
+
Method B
|
| 174 |
+
59
|
| 175 |
+
64
|
| 176 |
+
61
|
| 177 |
+
70
|
| 178 |
+
63
|
| 179 |
+
62
|
| 180 |
+
62
|
| 181 |
+
62
|
| 182 |
+
58
|
| 183 |
+
61
|
| 184 |
+
47
|
| 185 |
+
63
|
| 186 |
+
64
|
| 187 |
+
74
|
| 188 |
+
67
|
| 189 |
+
57
|
| 190 |
+
53
|
| 191 |
+
68
|
| 192 |
+
61
|
| 193 |
+
59
|
| 194 |
+
67
|
| 195 |
+
Language
|
| 196 |
+
ita
|
| 197 |
+
lit
|
| 198 |
+
lav
|
| 199 |
+
mkd
|
| 200 |
+
zlm
|
| 201 |
+
nld
|
| 202 |
+
nor
|
| 203 |
+
pol
|
| 204 |
+
por
|
| 205 |
+
ron
|
| 206 |
+
rus
|
| 207 |
+
slk
|
| 208 |
+
slv
|
| 209 |
+
alb
|
| 210 |
+
swe
|
| 211 |
+
tam
|
| 212 |
+
tgl
|
| 213 |
+
tur
|
| 214 |
+
ukr
|
| 215 |
+
vie
|
| 216 |
+
AVG
|
| 217 |
+
Method A
|
| 218 |
+
76
|
| 219 |
+
75
|
| 220 |
+
67
|
| 221 |
+
48
|
| 222 |
+
63
|
| 223 |
+
78
|
| 224 |
+
77
|
| 225 |
+
77
|
| 226 |
+
74
|
| 227 |
+
74
|
| 228 |
+
36
|
| 229 |
+
76
|
| 230 |
+
76
|
| 231 |
+
76
|
| 232 |
+
69
|
| 233 |
+
25
|
| 234 |
+
57
|
| 235 |
+
67
|
| 236 |
+
49
|
| 237 |
+
48
|
| 238 |
+
64.5
|
| 239 |
+
Method B
|
| 240 |
+
60
|
| 241 |
+
62
|
| 242 |
+
68
|
| 243 |
+
67
|
| 244 |
+
66
|
| 245 |
+
59
|
| 246 |
+
65
|
| 247 |
+
61
|
| 248 |
+
59
|
| 249 |
+
66
|
| 250 |
+
53
|
| 251 |
+
62
|
| 252 |
+
64
|
| 253 |
+
69
|
| 254 |
+
69
|
| 255 |
+
54
|
| 256 |
+
66
|
| 257 |
+
61
|
| 258 |
+
60
|
| 259 |
+
55
|
| 260 |
+
62.1
|
| 261 |
+
Table 1: Comparison of two methods from Rahimi et al. (2019).
|
| 262 |
+
as a default hub language, even though this might
|
| 263 |
+
hurt many languages (Anastasopoulos and Neubig,
|
| 264 |
+
2020). Perhaps if the practice of research was less
|
| 265 |
+
Anglocentric, different methods and techniques
|
| 266 |
+
would have become popular instead. Our work
|
| 267 |
+
is deeply related to issues like these. We show that
|
| 268 |
+
multilingual evaluation with an unbalanced selec-
|
| 269 |
+
tion of languages might cause similar symptoms.
|
| 270 |
+
Benchmarking.
|
| 271 |
+
Using benchmarks is a practice
|
| 272 |
+
that came under a lot of scrutiny in the NLP com-
|
| 273 |
+
munity recently. Benchmark evaluation was said
|
| 274 |
+
to encourage spurious data overfitting (Kavumba
|
| 275 |
+
et al., 2019), encourage metric gaming (Thomas
|
| 276 |
+
and Uminsky, 2020) or lead the research away from
|
| 277 |
+
general human-like linguistic intelligence (Linzen,
|
| 278 |
+
2020). Similarly, benchmarks are criticized for be-
|
| 279 |
+
ing predominantly focused on performance, while
|
| 280 |
+
neglecting several other important properties, e.g.
|
| 281 |
+
prediction cost or model robustness (Ethayarajh
|
| 282 |
+
and Jurafsky, 2020). Average in particular was
|
| 283 |
+
shown to have several issues with robustness that
|
| 284 |
+
can be addressed by using pair-wise instance evalu-
|
| 285 |
+
ation (Peyrard et al., 2021). To address these issues,
|
| 286 |
+
some benchmarks refuse to use aggregating scores
|
| 287 |
+
and instead report multiple metrics at the same time
|
| 288 |
+
leaving interpretation of the results to the reader.
|
| 289 |
+
Gehrmann et al. (2021) is one such benchmark,
|
| 290 |
+
which proposes to use visualizations to help the in-
|
| 291 |
+
tepretation. In this work, we also use visualizations
|
| 292 |
+
to similar effect.
|
| 293 |
+
3
|
| 294 |
+
Multilingual Evaluation Strategies
|
| 295 |
+
When comparing multilingual methods with non-
|
| 296 |
+
trivial number of languages, it is cognitively hard
|
| 297 |
+
to keep track of various linguistic aspects, such
|
| 298 |
+
as language families, writing systems, typologi-
|
| 299 |
+
cal properties, etc. Researchers often use various
|
| 300 |
+
simplifying strategies instead:
|
| 301 |
+
Aggregating
|
| 302 |
+
metrics.
|
| 303 |
+
Aggregating
|
| 304 |
+
metrics,
|
| 305 |
+
such as average performance or a number of
|
| 306 |
+
languages where a certain method achieves the
|
| 307 |
+
best results provide some information, but as
|
| 308 |
+
we illustrated in Figure 1 (a), they might not
|
| 309 |
+
tell the whole story.
|
| 310 |
+
By aggregating results
|
| 311 |
+
we lose important information about individual
|
| 312 |
+
languages and language families.
|
| 313 |
+
Commonly
|
| 314 |
+
used statistics usually do not take underlying
|
| 315 |
+
linguistic diversity into account. This might lead
|
| 316 |
+
to unwanted phenomena, such as bias in favor
|
| 317 |
+
of dominant language families.
|
| 318 |
+
The encoded
|
| 319 |
+
values of the aggregating metrics might not align
|
| 320 |
+
with the values we want to express. Average is
|
| 321 |
+
an example of utilitarianist world view, while
|
| 322 |
+
using minimal performance might be considered
|
| 323 |
+
to be a prioritarianist approach (Choudhury and
|
| 324 |
+
Deshpande, 2021). Even though analyzing the
|
| 325 |
+
|
| 326 |
+
values encoded in metrics is a step towards a fairer
|
| 327 |
+
evaluation, they still miss a more fine-grained
|
| 328 |
+
details of the results.
|
| 329 |
+
Aggregated metrics for different groups.
|
| 330 |
+
An-
|
| 331 |
+
other option is to calculate statistics for certain
|
| 332 |
+
linguistic families or groups. These are steps in
|
| 333 |
+
the right direction, as they provide a more fine-
|
| 334 |
+
grained picture, but there are still issues left. It is
|
| 335 |
+
not clear which families should be selected, e.g.
|
| 336 |
+
should we average all Indo-European languages
|
| 337 |
+
or should we average across subfamilies, such as
|
| 338 |
+
Slavic or Germanic. This selection is ultimately
|
| 339 |
+
opinionated and different selections might show us
|
| 340 |
+
different views of the results. In addition, aggregat-
|
| 341 |
+
ing across families might still hide variance within
|
| 342 |
+
these families. Grouping languages by the size of
|
| 343 |
+
available datasets (e.g. low resource vs. high re-
|
| 344 |
+
source) shows us how the models deal with data
|
| 345 |
+
scarcity, but the groups might still be linguistically
|
| 346 |
+
unbalanced.
|
| 347 |
+
Balanced language sampling.
|
| 348 |
+
Another option
|
| 349 |
+
is to construct a multilingual dataset so that it is
|
| 350 |
+
linguistically balanced. This process is called lan-
|
| 351 |
+
guage sampling (Rijkhoff et al., 1993; Miestamo
|
| 352 |
+
et al., 2016). In practice, this means that a small
|
| 353 |
+
number of representative languages is selected for
|
| 354 |
+
each family. The problem with dominant fami-
|
| 355 |
+
lies is solved because we control the number of
|
| 356 |
+
languages per family. However, selecting which
|
| 357 |
+
families should be represented and then selecting
|
| 358 |
+
languages within these families is again an opin-
|
| 359 |
+
ionated process. Different families and their sub-
|
| 360 |
+
families might have different degrees of diversity.
|
| 361 |
+
Different selections might favor different linguistic
|
| 362 |
+
properties and results might vary between them. It
|
| 363 |
+
is also not clear, how exhaustive given selection is,
|
| 364 |
+
i.e. how much of the linguistic variety has been
|
| 365 |
+
covered. Some of the existing works mention their
|
| 366 |
+
selection criteria: Longpre et al. (2020) count how
|
| 367 |
+
many speakers the selection covers, Clark et al.
|
| 368 |
+
(2020) use a set of selected typological proper-
|
| 369 |
+
ties, Ponti et al. (2020) use the so called variety
|
| 370 |
+
language sampling. Publishing the criteria allows
|
| 371 |
+
us to do a post-hoc analysis in the future to evaluate,
|
| 372 |
+
how well did these criteria work.
|
| 373 |
+
Qualitative analysis
|
| 374 |
+
In this paper, we argue that
|
| 375 |
+
qualitative analysis is an often overlooked, yet ir-
|
| 376 |
+
replaceable evaluation technique. In the following
|
| 377 |
+
section, we will present our case study of how to
|
| 378 |
+
perform qualitative analysis.
|
| 379 |
+
4
|
| 380 |
+
Case Study: Qualitative Analysis
|
| 381 |
+
through Visualization
|
| 382 |
+
In this section we show how to perform a quali-
|
| 383 |
+
tative analysis of multilingual results with a visu-
|
| 384 |
+
alization technique based on URIEL typographic
|
| 385 |
+
database.
|
| 386 |
+
We show that using this we can (1)
|
| 387 |
+
uncover linguistic biases in the results, and (2)
|
| 388 |
+
make sense of results from non-trivial number of
|
| 389 |
+
languages. As case study, we study results from
|
| 390 |
+
Rahimi et al. (2019). Our goal is not to evaluate
|
| 391 |
+
particular methods from this paper, but to demon-
|
| 392 |
+
strate how linguistically-informed analysis might
|
| 393 |
+
help researchers gain insights into their results. We
|
| 394 |
+
analyze the results from this paper not because we
|
| 395 |
+
want to criticize it, but because it is a well-written
|
| 396 |
+
paper that actually attempts to do multilingual eval-
|
| 397 |
+
uation for non-trivial number of languages with
|
| 398 |
+
significantly different methods. The linguistic bi-
|
| 399 |
+
ases we uncover are already partially discussed in
|
| 400 |
+
the paper. Here, we only show how to effectively
|
| 401 |
+
perform qualitative analysis and uncover these bi-
|
| 402 |
+
ases with appropriate visualization. Appendix A
|
| 403 |
+
shows similar analysis for another paper (Heinzer-
|
| 404 |
+
ling and Strube, 2019) where linguistic biases are
|
| 405 |
+
visible.
|
| 406 |
+
We use URIEL, a typological language database
|
| 407 |
+
that consists of 289 syntactic and phonological bi-
|
| 408 |
+
nary features for 3718 languages. We use UMAP
|
| 409 |
+
feature reduction algorithm (McInnes and Healy,
|
| 410 |
+
2018) to create a 2D typological language space.
|
| 411 |
+
This map is shown in Figure 1 (b). The map is inter-
|
| 412 |
+
active and allows for dynamic filtering of languages
|
| 413 |
+
and families, as well as inspection of individual
|
| 414 |
+
languages and their properties.1 Each point is one
|
| 415 |
+
language and selected language families are color-
|
| 416 |
+
coded in the figure. Even though URIEL features
|
| 417 |
+
used for dimensionality reduction do not contain in-
|
| 418 |
+
formation about language families, genealogically
|
| 419 |
+
close languages naturally form clusters in our vi-
|
| 420 |
+
sualization. Certain geographical relations are cap-
|
| 421 |
+
tured as well, e.g. Sudanic and Chadic languages
|
| 422 |
+
are neighboring clusters, despite being from differ-
|
| 423 |
+
ent language families. This evokes the linguistic
|
| 424 |
+
tradition of grouping languages according to the
|
| 425 |
+
regions and macroregions. This shows that our vi-
|
| 426 |
+
sualization is able to capture both intrafamiliar and
|
| 427 |
+
interfamiliar similarities of languages and is thus
|
| 428 |
+
appropriate for our use-case.
|
| 429 |
+
We visualize results from Rahimi et al. (2019)
|
| 430 |
+
on this linguistic map. Rahimi et al. use Wikipedia-
|
| 431 |
+
1Code available at GitHub
|
| 432 |
+
|
| 433 |
+
based corpus for NER, and they compare various
|
| 434 |
+
cross-lingual transfer learning algorithms for 41
|
| 435 |
+
languages. They use an unbalanced set of lan-
|
| 436 |
+
guages, where the three most dominant language
|
| 437 |
+
families – Germanic, Italic and Slavic – make up
|
| 438 |
+
55% of all languages. See Appendix A for more
|
| 439 |
+
details about the paper. We use our URIEL map to
|
| 440 |
+
visualize a comparison between a pair of methods
|
| 441 |
+
on all 41 languages from Table 1. In Figure 1 (c) we
|
| 442 |
+
compare two methods – Method A – cross-lingual
|
| 443 |
+
transfer learning methods using multiple source lan-
|
| 444 |
+
guages (average performance 64.5), and seemingly
|
| 445 |
+
worse Method B – a low-resource training with-
|
| 446 |
+
out any form of cross-lingual supervision (average
|
| 447 |
+
performance 62.1). We use the same URIEL map,
|
| 448 |
+
but we superimpose the relative performance of the
|
| 449 |
+
two methods as colored columns. Orange columns
|
| 450 |
+
on this map show languages where Method A per-
|
| 451 |
+
forms better, while blue columns show the same for
|
| 452 |
+
Method B. Height of each column shows how big
|
| 453 |
+
the relative difference in performance is between
|
| 454 |
+
the two methods. I.e. taller orange columns mean
|
| 455 |
+
dominant A, taller blue columns mean dominant B.
|
| 456 |
+
We can now clearly see that there is a pattern in
|
| 457 |
+
the location of the colored columns. Using aver-
|
| 458 |
+
age as evaluation measure, Method A seems better
|
| 459 |
+
overall. Here we can see that it is only better in
|
| 460 |
+
one particular cluster of languages – the cluster of
|
| 461 |
+
orange columns. All these are related European
|
| 462 |
+
languages. Most of them are Germanic, Italic or
|
| 463 |
+
Slavic, with some exceptions being languages that
|
| 464 |
+
are not Indo-European, but are nevertheless geo-
|
| 465 |
+
graphical neighbors, such as Hungarian. On the
|
| 466 |
+
other hand, all the non-European languages actu-
|
| 467 |
+
ally prefer Method B. These are the blue columns
|
| 468 |
+
scattered in the rest of the space that consists of
|
| 469 |
+
languages such as Arabic (Semitic), Chinese (Sino-
|
| 470 |
+
Tibetan) or Tamil (Dravidian).
|
| 471 |
+
This shows important fact about the two methods
|
| 472 |
+
that was hidden by using average. Cross-lingual su-
|
| 473 |
+
pervision seemed to have better performance, but it
|
| 474 |
+
has better performance only in the dominant cluster
|
| 475 |
+
of similar languages where the cross-lingual super-
|
| 476 |
+
vision is more viable. Other languages, would actu-
|
| 477 |
+
ally prefer using monolingual low-resource learn-
|
| 478 |
+
ing, as they are not able to learn from other lan-
|
| 479 |
+
guages that easily. In this case, average is overesti-
|
| 480 |
+
mating the value of cross-lingual learning for non-
|
| 481 |
+
European languages. This overestimation might
|
| 482 |
+
cause harm to these languages.
|
| 483 |
+
We can also see that there are some exceptions –
|
| 484 |
+
the blue columns in the orange cluster. These ex-
|
| 485 |
+
ceptions are Greek, Russian, Macedonian, Bulgar-
|
| 486 |
+
ian and Ukrainian – all Indo-European languages
|
| 487 |
+
that use non-Latin scripts. In this case, different
|
| 488 |
+
writing systems are probably cause of additional
|
| 489 |
+
linguistic bias. It might be hard to notice this pat-
|
| 490 |
+
tern by simply looking at the table of results, but
|
| 491 |
+
here we can quickly identify the languages as out-
|
| 492 |
+
liers and then it is easy to realize what they have in
|
| 493 |
+
common.
|
| 494 |
+
Note that we do not expect to see this level of
|
| 495 |
+
linguistic bias in most papers and we have cherry-
|
| 496 |
+
picked this particular methods from this particu-
|
| 497 |
+
lar paper because they demonstrate the case when
|
| 498 |
+
the linguistic bias in the results is the most obvi-
|
| 499 |
+
ous. This is caused mainly by unbalanced selection
|
| 500 |
+
of languages on Wikipedia and in a sense unfair
|
| 501 |
+
comparison of cross-lingual supervision with low
|
| 502 |
+
resource learning.
|
| 503 |
+
5
|
| 504 |
+
Conclusions
|
| 505 |
+
Multilinguality in NLP is becoming more common
|
| 506 |
+
and methodological practice is sometimes lagging
|
| 507 |
+
behind (Artetxe et al., 2020; Keung et al., 2020;
|
| 508 |
+
Bender, 2011). Making progress will be inherently
|
| 509 |
+
hard without proper evaluation methodology. In
|
| 510 |
+
this work, we argue for necessity for qualitative
|
| 511 |
+
results analysis and we showed how to use such
|
| 512 |
+
analysis to improve the evaluation with interactive
|
| 513 |
+
visualizations. In our case study, we were able to
|
| 514 |
+
uncover linguistic biases in published results.
|
| 515 |
+
Considering the practice in machine learning and
|
| 516 |
+
NLP, it might be tempting to reduce a multilingual
|
| 517 |
+
method performance to a single number. However,
|
| 518 |
+
we believe that intricacies of multilingual evalua-
|
| 519 |
+
tion can not be reduced so easily. There are too
|
| 520 |
+
many different dimensions that need to be taken
|
| 521 |
+
into consideration and NLP researchers should un-
|
| 522 |
+
derstand these dimensions. We believe that appro-
|
| 523 |
+
priate level of training in various linguistic fields,
|
| 524 |
+
such as typology or comparative linguistics, is nec-
|
| 525 |
+
essary for proper understanding of multilingual
|
| 526 |
+
results and for proper qualitative analysis. We ar-
|
| 527 |
+
gue that qualitative analysis is an oft overlooked
|
| 528 |
+
approach to results analysis that should be utilized
|
| 529 |
+
more to prevent various distortions in how we un-
|
| 530 |
+
derstand linguistic implications of our results.
|
| 531 |
+
6
|
| 532 |
+
Ethical Considerations
|
| 533 |
+
Much of current NLP research is focused on only a
|
| 534 |
+
small handful of languages. Communities of some
|
| 535 |
+
|
| 536 |
+
language users are left behind, as a result of data
|
| 537 |
+
scarcity. We believe that our paper might have
|
| 538 |
+
positive societal impact. It focuses on the issues
|
| 539 |
+
of these marginalized languages and communities.
|
| 540 |
+
Following our recommendations might lead to a
|
| 541 |
+
more diverse and fair multilingual evaluation both
|
| 542 |
+
in research and in industry. This might in turn led to
|
| 543 |
+
better models, applications and ultimately quality
|
| 544 |
+
of life changes for some.
|
| 545 |
+
Acknowledgments
|
| 546 |
+
This research was partially supported by DisAi,
|
| 547 |
+
a project funded by Horizon Europe under GA No.
|
| 548 |
+
101079164.
|
| 549 |
+
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Computational Linguistics.
|
| 732 |
+
Matúš Pikuliak, Marián Šimko, and Mária Bieliková.
|
| 733 |
+
2021.
|
| 734 |
+
Cross-lingual learning for text process-
|
| 735 |
+
ing: A survey. Expert Systems with Applications,
|
| 736 |
+
165:113765.
|
| 737 |
+
Edoardo Maria Ponti, Goran Glavaš, Olga Majewska,
|
| 738 |
+
Qianchu Liu, Ivan Vuli´c, and Anna Korhonen. 2020.
|
| 739 |
+
XCOPA: A multilingual dataset for causal common-
|
| 740 |
+
sense reasoning. In Proceedings of the 2020 Con-
|
| 741 |
+
ference on Empirical Methods in Natural Language
|
| 742 |
+
Processing (EMNLP), pages 2362–2376, Online. As-
|
| 743 |
+
sociation for Computational Linguistics.
|
| 744 |
+
Edoardo Maria Ponti, Helen O’Horan, Yevgeni Berzak,
|
| 745 |
+
Ivan Vuli´c, Roi Reichart, Thierry Poibeau, Ekaterina
|
| 746 |
+
Shutova, and Anna Korhonen. 2019. Modeling lan-
|
| 747 |
+
guage variation and universals: A survey on typo-
|
| 748 |
+
logical linguistics for natural language processing.
|
| 749 |
+
Computational Linguistics, 45(3):559–601.
|
| 750 |
+
Afshin Rahimi, Yuan Li, and Trevor Cohn. 2019. Mas-
|
| 751 |
+
sively multilingual transfer for NER.
|
| 752 |
+
In Proceed-
|
| 753 |
+
ings of the 57th Annual Meeting of the Association
|
| 754 |
+
for Computational Linguistics, pages 151–164, Flo-
|
| 755 |
+
rence, Italy. Association for Computational Linguis-
|
| 756 |
+
tics.
|
| 757 |
+
Jan Rijkhoff, Dik Bakker, Kees Hengeveld, and Pe-
|
| 758 |
+
ter Kahrel. 1993.
|
| 759 |
+
A method of language sam-
|
| 760 |
+
pling. Studies in Language. International Journal
|
| 761 |
+
sponsored by the Foundation “Foundations of Lan-
|
| 762 |
+
guage”, 17(1):169–203.
|
| 763 |
+
Sebastian Ruder, Ivan Vulic, and Anders Søgaard.
|
| 764 |
+
2019. A survey of cross-lingual word embedding
|
| 765 |
+
models. Journal of Artificial Intelligence Research,
|
| 766 |
+
65:569–631.
|
| 767 |
+
Rachel Thomas and David Uminsky. 2020. The prob-
|
| 768 |
+
lem with metrics is a fundamental problem for AI.
|
| 769 |
+
CoRR, abs/2002.08512.
|
| 770 |
+
|
| 771 |
+
A
|
| 772 |
+
Details of Analysed Papers
|
| 773 |
+
In this appendix, we provide additional information
|
| 774 |
+
about papers we analysed.
|
| 775 |
+
A.1
|
| 776 |
+
Rahimi et al.
|
| 777 |
+
This is the paper we used for demonstration in the
|
| 778 |
+
main paper in Section 4. We use results reported in
|
| 779 |
+
Table 4 in their paper. The languages they use are
|
| 780 |
+
listed here in Table 2. We can see the apparent dom-
|
| 781 |
+
inance of Indo-European languages. There are 14
|
| 782 |
+
different methods listed in their paper. We compare
|
| 783 |
+
the results for these methods in Figure 2. There we
|
| 784 |
+
can see how the average results for individual meth-
|
| 785 |
+
ods compare with the average results for non-GIS
|
| 786 |
+
(Germanic-Italic-Slavic) languages. The numbers
|
| 787 |
+
correspond to the order of methods listed in the
|
| 788 |
+
original paper. The two methods compared in Fig-
|
| 789 |
+
ure 1 (c) are shown as blue and orange, respectively.
|
| 790 |
+
The orange Method A is BEAtok in the original pa-
|
| 791 |
+
per. The blue Method B is called LSup. We can see
|
| 792 |
+
the linguistic bias with this simplistic view as well.
|
| 793 |
+
All the cross-lingual learning based methods have
|
| 794 |
+
worse non-GIS results than methods that do not use
|
| 795 |
+
cross-lingual learning (methods 1 and 2). However,
|
| 796 |
+
this analysis can not replace the visualization we
|
| 797 |
+
propose in Section 4. It provides a GIS-centered
|
| 798 |
+
view, but it can not capture other sources of bias.
|
| 799 |
+
For example, it does not show various outliers that
|
| 800 |
+
were seen in the visualization, such as Uralic lan-
|
| 801 |
+
guages that behave similarly to GIS languages, or
|
| 802 |
+
Slavic languages with Cyrilic alphabet that behave
|
| 803 |
+
differently than other Slavic languages.
|
| 804 |
+
A.2
|
| 805 |
+
Heinzerling and Strube
|
| 806 |
+
Similar linguistic biases can be seen in Heinzer-
|
| 807 |
+
ling and Strube as well. They evaluate various
|
| 808 |
+
representations performance on POS tagging and
|
| 809 |
+
NER. In Figure 3 we compare POS accuracy of a
|
| 810 |
+
multilingual model with a shared embedding vocab-
|
| 811 |
+
ulary (average performance 96.6, MultiBPEmb
|
| 812 |
+
+char +finetune in the original paper) and a
|
| 813 |
+
simple BiLSTM baseline with no transfer super-
|
| 814 |
+
vision (average performance 96.4, BiLSTM in the
|
| 815 |
+
original paper). Orange columns are for languages
|
| 816 |
+
that prefer the multilingual model, blue columns
|
| 817 |
+
prefer the baseline. In this case, almost all orange
|
| 818 |
+
columns are in fact GIS languages. Other lan-
|
| 819 |
+
guages are having significantly worse results with
|
| 820 |
+
this method and most of them actually prefer the
|
| 821 |
+
simple baseline with no cross-lingual supervision.
|
| 822 |
+
This shows the limitations of proposed multilingual
|
| 823 |
+
ISO
|
| 824 |
+
Language
|
| 825 |
+
Subfamily
|
| 826 |
+
Family
|
| 827 |
+
bul
|
| 828 |
+
Bulgarian
|
| 829 |
+
Slavic
|
| 830 |
+
Indo-European
|
| 831 |
+
bos
|
| 832 |
+
Bosnian
|
| 833 |
+
ces
|
| 834 |
+
Czech
|
| 835 |
+
hrv
|
| 836 |
+
Croatian
|
| 837 |
+
mkd
|
| 838 |
+
Macedonian
|
| 839 |
+
pol
|
| 840 |
+
Polish
|
| 841 |
+
rus
|
| 842 |
+
Russian
|
| 843 |
+
slk
|
| 844 |
+
Slovak
|
| 845 |
+
slv
|
| 846 |
+
Slovenian
|
| 847 |
+
ukr
|
| 848 |
+
Ukrainian
|
| 849 |
+
afr
|
| 850 |
+
Afrikkans
|
| 851 |
+
Germanic
|
| 852 |
+
dan
|
| 853 |
+
Danish
|
| 854 |
+
deu
|
| 855 |
+
German
|
| 856 |
+
nld
|
| 857 |
+
Dutch
|
| 858 |
+
nor
|
| 859 |
+
Norwegian
|
| 860 |
+
swe
|
| 861 |
+
Swedish
|
| 862 |
+
cat
|
| 863 |
+
Catalan
|
| 864 |
+
Italic
|
| 865 |
+
fra
|
| 866 |
+
French
|
| 867 |
+
ita
|
| 868 |
+
Italian
|
| 869 |
+
por
|
| 870 |
+
Portugese
|
| 871 |
+
rom
|
| 872 |
+
Romanina
|
| 873 |
+
spa
|
| 874 |
+
Spanish
|
| 875 |
+
ben
|
| 876 |
+
Bengali
|
| 877 |
+
Indo-Iranian
|
| 878 |
+
hin
|
| 879 |
+
Hindi
|
| 880 |
+
pes
|
| 881 |
+
Iranian Persian
|
| 882 |
+
lit
|
| 883 |
+
Lithuanian
|
| 884 |
+
Baltic
|
| 885 |
+
lav
|
| 886 |
+
Latvian
|
| 887 |
+
ell
|
| 888 |
+
Greek
|
| 889 |
+
alb
|
| 890 |
+
Albanian
|
| 891 |
+
est
|
| 892 |
+
Estonian
|
| 893 |
+
Uralic
|
| 894 |
+
fin
|
| 895 |
+
Finnish
|
| 896 |
+
hun
|
| 897 |
+
Hungarian
|
| 898 |
+
ind
|
| 899 |
+
Indonesian
|
| 900 |
+
Austronesian
|
| 901 |
+
tgl
|
| 902 |
+
Tagalog
|
| 903 |
+
zlm
|
| 904 |
+
Malay
|
| 905 |
+
arb
|
| 906 |
+
Standard Arabic
|
| 907 |
+
Afro-Asiatic
|
| 908 |
+
heb
|
| 909 |
+
Hebrew
|
| 910 |
+
vie
|
| 911 |
+
Vietnamese
|
| 912 |
+
Austroasiatic
|
| 913 |
+
tam
|
| 914 |
+
Tamil
|
| 915 |
+
Davidian
|
| 916 |
+
tur
|
| 917 |
+
Turkish
|
| 918 |
+
Turkic
|
| 919 |
+
Table 2: Languages used in Rahimi et al..
|
| 920 |
+
ISO
|
| 921 |
+
Language
|
| 922 |
+
Subfamily
|
| 923 |
+
Family
|
| 924 |
+
dan
|
| 925 |
+
Danish
|
| 926 |
+
Germanic
|
| 927 |
+
Indo-European
|
| 928 |
+
deu
|
| 929 |
+
German
|
| 930 |
+
eng
|
| 931 |
+
English
|
| 932 |
+
nld
|
| 933 |
+
Dutch
|
| 934 |
+
nor
|
| 935 |
+
Norwegian
|
| 936 |
+
swe
|
| 937 |
+
Swedish
|
| 938 |
+
bul
|
| 939 |
+
Bulgarian
|
| 940 |
+
Slavic
|
| 941 |
+
ces
|
| 942 |
+
Czech
|
| 943 |
+
hrv
|
| 944 |
+
Croatian
|
| 945 |
+
pol
|
| 946 |
+
Polish
|
| 947 |
+
slv
|
| 948 |
+
Slovenian
|
| 949 |
+
fra
|
| 950 |
+
Frech
|
| 951 |
+
Italic
|
| 952 |
+
ita
|
| 953 |
+
Italian
|
| 954 |
+
por
|
| 955 |
+
Portugese
|
| 956 |
+
spa
|
| 957 |
+
Spanish
|
| 958 |
+
hin
|
| 959 |
+
Hindi
|
| 960 |
+
Indo-Iranian
|
| 961 |
+
pes
|
| 962 |
+
Iranian Persian
|
| 963 |
+
eus
|
| 964 |
+
Basque
|
| 965 |
+
Isolate
|
| 966 |
+
fin
|
| 967 |
+
Finnish
|
| 968 |
+
Uralic
|
| 969 |
+
heb
|
| 970 |
+
Hebrew
|
| 971 |
+
Afro-Asiatic
|
| 972 |
+
ind
|
| 973 |
+
Indonesian
|
| 974 |
+
Austronesian
|
| 975 |
+
Table 3: Languages used in Heinzerling and Strube.
|
| 976 |
+
|
| 977 |
+
50
|
| 978 |
+
60
|
| 979 |
+
70
|
| 980 |
+
80
|
| 981 |
+
90
|
| 982 |
+
Total average
|
| 983 |
+
40
|
| 984 |
+
50
|
| 985 |
+
60
|
| 986 |
+
70
|
| 987 |
+
80
|
| 988 |
+
90
|
| 989 |
+
Non-GIS average
|
| 990 |
+
0
|
| 991 |
+
1
|
| 992 |
+
2
|
| 993 |
+
3
|
| 994 |
+
4
|
| 995 |
+
5
|
| 996 |
+
6
|
| 997 |
+
7
|
| 998 |
+
8
|
| 999 |
+
9
|
| 1000 |
+
10
|
| 1001 |
+
11
|
| 1002 |
+
12
|
| 1003 |
+
13
|
| 1004 |
+
Rahimi et al.
|
| 1005 |
+
95.25 95.50 95.75 96.00 96.25 96.50 96.75
|
| 1006 |
+
Total average
|
| 1007 |
+
94.5
|
| 1008 |
+
95.0
|
| 1009 |
+
95.5
|
| 1010 |
+
96.0
|
| 1011 |
+
Non-GIS average
|
| 1012 |
+
0
|
| 1013 |
+
1
|
| 1014 |
+
2
|
| 1015 |
+
3
|
| 1016 |
+
4
|
| 1017 |
+
5
|
| 1018 |
+
6
|
| 1019 |
+
7
|
| 1020 |
+
8
|
| 1021 |
+
9
|
| 1022 |
+
10
|
| 1023 |
+
Heinzerling and Strube
|
| 1024 |
+
Figure 2: Comparison of method performance. The re-
|
| 1025 |
+
lation between global average and average on non-GIS
|
| 1026 |
+
languages is shown. Each point represents one method
|
| 1027 |
+
from the papers.
|
| 1028 |
+
supervision for outlier languages.
|
| 1029 |
+
We use results reported in Table 5 in their paper.
|
| 1030 |
+
The languages they use are listed here in Table 3.
|
| 1031 |
+
Again, we can see an apparent dominance of GIS
|
| 1032 |
+
languages. There are 11 different methods listed in
|
| 1033 |
+
their paper. We omitted results for additional 6 low
|
| 1034 |
+
resource languages reported in Table 7, because
|
| 1035 |
+
only 4 out of 11 methods were used there. We
|
| 1036 |
+
compare the results for these methods in Figure 2,
|
| 1037 |
+
similarly as in the previous paper. The orange point
|
| 1038 |
+
is the multilingual model, the blue point is the base-
|
| 1039 |
+
line. Now we can see that the BiLSTM baseline is
|
| 1040 |
+
actually the best performing method for non-GIS
|
| 1041 |
+
languages.
|
| 1042 |
+
B
|
| 1043 |
+
Hyperparameters
|
| 1044 |
+
We use UMAP python library2 with the following
|
| 1045 |
+
hyperparameters:
|
| 1046 |
+
2umap-learn.readthedocs.io
|
| 1047 |
+
Figure 3: Comparison of two methods from Heinzer-
|
| 1048 |
+
ling and Strube.
|
| 1049 |
+
• Number of neighbours (n_neighbors): 15
|
| 1050 |
+
• Distance metric (metric): cosine
|
| 1051 |
+
• Minimal distance (min_dist): 0.5
|
| 1052 |
+
• Random see (random_state): 1
|
| 1053 |
+
C
|
| 1054 |
+
Additional Visualizations
|
| 1055 |
+
In this Section we show several additional possibil-
|
| 1056 |
+
ities of using URIEL map of languages to visualize
|
| 1057 |
+
results from multilingual evaluation. Our goal here
|
| 1058 |
+
is to propose additional techniques that can be used
|
| 1059 |
+
for qualitative analysis apart from the comparison
|
| 1060 |
+
of two methods used in Figure 1 in the main body
|
| 1061 |
+
of this paper. This is not an exhaustive list of vi-
|
| 1062 |
+
sualizations. We believe that many other types of
|
| 1063 |
+
visualization can be done using this type of qualita-
|
| 1064 |
+
tive analysis, based on the needs and requirements
|
| 1065 |
+
of the user.
|
| 1066 |
+
In Figure 4 we show how to compare more than
|
| 1067 |
+
two methods by visualizing the performance for
|
| 1068 |
+
each method separately. We have created a sepa-
|
| 1069 |
+
rate plot for three methods and we can compare
|
| 1070 |
+
their performance visually. We can see that HSup
|
| 1071 |
+
method has overall stable high performance. LSup
|
| 1072 |
+
has worse performance, but its still quite balanced.
|
| 1073 |
+
Finally, BWET has similar performance as LSup,
|
| 1074 |
+
but we can see that there are regions where it fails,
|
| 1075 |
+
e.g. the languages in the rightmost part of the figure
|
| 1076 |
+
have visibly worse performance.
|
| 1077 |
+
In Figure 5 we show yet another type of visu-
|
| 1078 |
+
alization. In this case, we simply visualize what
|
| 1079 |
+
method is the best performing for each language.
|
| 1080 |
+
|
| 1081 |
+
HSup
|
| 1082 |
+
20
|
| 1083 |
+
40
|
| 1084 |
+
60
|
| 1085 |
+
80
|
| 1086 |
+
LSup
|
| 1087 |
+
BWET
|
| 1088 |
+
Figure 4: Comparison of multiple methods using size to mark method performance for individual languages. HSup,
|
| 1089 |
+
LSup and BWET are methods reported in (Rahimi et al., 2019).
|
| 1090 |
+
LSup
|
| 1091 |
+
RaReuns
|
| 1092 |
+
BEAent
|
| 1093 |
+
unsx2
|
| 1094 |
+
BEAent
|
| 1095 |
+
uns
|
| 1096 |
+
Figure 5: The best performing methods for various lan-
|
| 1097 |
+
guages.
|
| 1098 |
+
We compare methods using crosslingual super-
|
| 1099 |
+
vision and low-resource training (LSup). From
|
| 1100 |
+
seven methods, only four achieved the best per-
|
| 1101 |
+
formance for at least one language and those are
|
| 1102 |
+
shown in the Figure. Again, we can see similar
|
| 1103 |
+
picture as before. One method (BEAent
|
| 1104 |
+
uns×2) is
|
| 1105 |
+
the best performing method taking average into
|
| 1106 |
+
account. However, in this visualization we can
|
| 1107 |
+
see that it is actually the best performing method
|
| 1108 |
+
only in the dominant cluster of European languages.
|
| 1109 |
+
Elsewhere, other methods perform better.
|
| 1110 |
+
|
GNAzT4oBgHgl3EQfUfzc/content/tmp_files/load_file.txt
ADDED
|
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See raw diff
|
|
|
HtFLT4oBgHgl3EQfIS87/content/tmp_files/2301.11999v1.pdf.txt
ADDED
|
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|
| 1 |
+
Particle-Number Threshold for Non-Abelian Geometric Phases
|
| 2 |
+
Julien Pinske, Vincent Burgtorf, and Stefan Scheel∗
|
| 3 |
+
Institut für Physik, Universität Rostock, Albert-Einstein–Straße 23-24, D-18059 Rostock, Germany
|
| 4 |
+
(Dated: January 31, 2023)
|
| 5 |
+
When a quantum state traverses a path, while being under the influence of a gauge potential, it
|
| 6 |
+
acquires a geometric phase that is often more than just a scalar quantity. The variety of unitary
|
| 7 |
+
transformations that can be realised by this form of parallel transport depends crucially on the
|
| 8 |
+
number of particles involved in the evolution. Here, we introduce a particle-number threshold (PNT)
|
| 9 |
+
that assesses a system’s capabilities to perform purely geometric manipulations of quantum states.
|
| 10 |
+
This threshold gives the minimal number of particles necessary to fully exploit a system’s potential
|
| 11 |
+
to generate non-Abelian geometric phases.
|
| 12 |
+
Therefore, the PNT might be useful for evaluating
|
| 13 |
+
the resource demands of a holonomic quantum computer. We benchmark our findings on bosonic
|
| 14 |
+
systems relevant to linear and nonlinear quantum optics.
|
| 15 |
+
I.
|
| 16 |
+
INTRODUCTION
|
| 17 |
+
The evolution of a quantum state,
|
| 18 |
+
in the pres-
|
| 19 |
+
ence of some potential, is completely determined by
|
| 20 |
+
Schrödinger’s equation which incorporates aspects such
|
| 21 |
+
as the system’s spectrum, or the overall evolution time. If
|
| 22 |
+
the system undergoes slow (adiabatic) changes, the evolv-
|
| 23 |
+
ing state remains unaffected by these dynamical contribu-
|
| 24 |
+
tions. Instead, its wave function acquires a phase factor
|
| 25 |
+
that only depends on the geometry of the path the quan-
|
| 26 |
+
tum state has traversed. This was first noticed by Berry
|
| 27 |
+
[1] who pointed out that, unlike dynamical phases, a ge-
|
| 28 |
+
ometric phase cannot be removed by a rescaling of the
|
| 29 |
+
energy (gauge transformation).
|
| 30 |
+
A famous example for
|
| 31 |
+
this is the Aharonov-Bohm effect [2], in which the wave
|
| 32 |
+
function of an electron traveling around a solenoidal mag-
|
| 33 |
+
netic field picks up a phase proportional to the magnetic
|
| 34 |
+
flux through the surface enclosed by the trajectory of the
|
| 35 |
+
electron. Pancharatnam studied the phenomenon in the
|
| 36 |
+
context of classical optics [3], where it manifests itself in
|
| 37 |
+
states of polarisation. It was pointed out by Simon [4]
|
| 38 |
+
that this purely geometric signature of a quantum evo-
|
| 39 |
+
lution has to be attributed to parallel transport of the
|
| 40 |
+
state vector along a path in a (projective) Hilbert space.
|
| 41 |
+
If a quantum system supports a d-fold degenerate sub-
|
| 42 |
+
space H0 with eigenstates |ψa⟩ (a = 1, . . . , d), an initially
|
| 43 |
+
prepared wave packet generically evolves into a superpo-
|
| 44 |
+
sition of the |ψa⟩ when undergoing adiabatic changes,
|
| 45 |
+
that is without population transfer to states of different
|
| 46 |
+
energy [5]. Wilzeck and Zee [6] associated such degen-
|
| 47 |
+
eracy of the spectrum with the possibility of emerging
|
| 48 |
+
non-Abelian (i.e., noncommuting) gauge potentials. In
|
| 49 |
+
this case, the state after a time period T does not only
|
| 50 |
+
acquire a (scalar) geometric phase but differs from the
|
| 51 |
+
initial one by a unitary d × d matrix.
|
| 52 |
+
If the Hamiltonian of the system is expressed through a
|
| 53 |
+
set of physically accessible parameters {κµ}µ that change
|
| 54 |
+
cyclically, i.e., κµ(0) = κµ(T), the time evolution is asso-
|
| 55 |
+
ciated with a closed path γ in the parameter space M .
|
| 56 |
+
∗ stefan.scheel@uni-rostock.de
|
| 57 |
+
The time evolution then takes the form of a quantum
|
| 58 |
+
holonomy (non-Abelian geometric phase) [6]
|
| 59 |
+
UA(γ) = ˆPexp
|
| 60 |
+
� ˛
|
| 61 |
+
γ
|
| 62 |
+
A
|
| 63 |
+
�
|
| 64 |
+
,
|
| 65 |
+
(1)
|
| 66 |
+
where A = �
|
| 67 |
+
µ Aµdκµ is the adiabatic connection (non-
|
| 68 |
+
Abelian gauge potential).
|
| 69 |
+
Depending on the physical
|
| 70 |
+
platform, the {κµ}µ might include external driving fields,
|
| 71 |
+
subsystem couplings, or hopping probabilities between
|
| 72 |
+
different states. Due to the generally noncommuting na-
|
| 73 |
+
ture of the connection, i.e., [Aµ, Aν] ̸= 0, the integration
|
| 74 |
+
in Eq. (1) has to be performed with respect to the path
|
| 75 |
+
ordering ˆP. The matrix-valued components of A can be
|
| 76 |
+
directly calculated from the eigenstates of the system,
|
| 77 |
+
i.e.,
|
| 78 |
+
(Aµ)ab = ⟨ψb| ∂µ |ψa⟩ ,
|
| 79 |
+
∂µ = ∂/∂κµ.
|
| 80 |
+
(2)
|
| 81 |
+
By traversing different loops in M one can potentially ac-
|
| 82 |
+
cess a variety of different unitaries UA(γ). The set of all
|
| 83 |
+
such transformations spans the holonomy group Hol(A).
|
| 84 |
+
It is a subset of the unitary group U(d). In addition to
|
| 85 |
+
their frequent occurrence in lattice-gauge theory [7] and
|
| 86 |
+
loop-quantum gravity [8], holonomy groups turn out to
|
| 87 |
+
be a crucial ingredient for geometric [9, 10] and topologi-
|
| 88 |
+
cal quantum computation [11], where they constitute the
|
| 89 |
+
fundamental gate set from which quantum algorithms are
|
| 90 |
+
to be implemented.
|
| 91 |
+
The question of how many different unitaries can be
|
| 92 |
+
harnessed by driving loops through M is therefore closely
|
| 93 |
+
related to computational universality [12], which holds
|
| 94 |
+
if Hol(A) = U(d). Not only does this require a d-fold
|
| 95 |
+
degenerate subspace, but a large parameter space as well
|
| 96 |
+
[9]. More recently, it was observed that the number of
|
| 97 |
+
particles prepared in the subspace H0 might drastically
|
| 98 |
+
alter the form of the holonomy UA(γ) [13–15]. This is
|
| 99 |
+
because the corresponding eigenstates |ψa⟩ can differ in
|
| 100 |
+
their particle number. In this work, quantum holonomies
|
| 101 |
+
are studied in relation to the number of particles involved
|
| 102 |
+
in the evolution. In the following, this issue is motivated
|
| 103 |
+
through an illustrative example.
|
| 104 |
+
arXiv:2301.11999v1 [quant-ph] 27 Jan 2023
|
| 105 |
+
|
| 106 |
+
2
|
| 107 |
+
A.
|
| 108 |
+
Λ-scheme of bosonic modes
|
| 109 |
+
Consider a chain of three bosonic modes [Fig. 1 (a)].
|
| 110 |
+
The outer modes ˆa± experience complex next-neighbour
|
| 111 |
+
couplings κ± to the central mode ˆac. The Hamiltonian
|
| 112 |
+
of the system reads
|
| 113 |
+
ˆH = κ+ˆa+ˆa†
|
| 114 |
+
c + κ−ˆacˆa†
|
| 115 |
+
− + H.c..
|
| 116 |
+
(3)
|
| 117 |
+
Here, ˆa†
|
| 118 |
+
k and ˆak denote the bosonic creation and anni-
|
| 119 |
+
hilation operators, respectively, and H.c. stands for the
|
| 120 |
+
Hermitian conjugate. The Hamiltonian (3) is the bosonic
|
| 121 |
+
counterpart of an atomic three-level system in Λ configu-
|
| 122 |
+
ration [16]. Such systems are of practical interest as they
|
| 123 |
+
describe linear-optical multiport systems [17] and can be
|
| 124 |
+
designed, for instance, in terms of integrated photonic
|
| 125 |
+
waveguides [18, 19].
|
| 126 |
+
Suppose a single photon is injected into one of the
|
| 127 |
+
outer modes of the optical setup, with couplings κ±(t)
|
| 128 |
+
varying slowly compared to the minimal energy gap
|
| 129 |
+
�
|
| 130 |
+
|κ+|2 + |κ−|2 > 0 (level crossing neglected).
|
| 131 |
+
In the
|
| 132 |
+
adiabatic limit, the photon remains in the zero-eigenvalue
|
| 133 |
+
eigenstate (aka dark state)
|
| 134 |
+
|D⟩ = sin θ |1+⟩ − cos θeiϕ |1−⟩ ,
|
| 135 |
+
where tan θ = |κ−|/|κ+|, ϕ = arg(κ+), and |1±⟩ = ˆa†
|
| 136 |
+
± |0⟩
|
| 137 |
+
with |0⟩ denoting the three-mode vacuum. Here, the con-
|
| 138 |
+
nection Aϕ = i cos2 θ is Abelian (while Aθ = 0). After
|
| 139 |
+
traversing a closed path γ in the (θ, ϕ) plane, the output
|
| 140 |
+
state |Ψ(T)⟩ = eiφ(γ) |Ψ(0)⟩ picks up a geometric phase
|
| 141 |
+
φ(γ) =
|
| 142 |
+
¨
|
| 143 |
+
D
|
| 144 |
+
sin(2θ)dϕdθ,
|
| 145 |
+
(4)
|
| 146 |
+
which depends on the area D enclosed by the loop γ.
|
| 147 |
+
Interestingly, injecting a second (indistinguishable)
|
| 148 |
+
photon into the setup, leads to the two dark states
|
| 149 |
+
|D1⟩ = sin2 θ |2+⟩ −
|
| 150 |
+
√
|
| 151 |
+
2 sin θ cos θeiϕ |1+1−⟩
|
| 152 |
+
+ cos2 θe2iϕ |2−⟩ ,
|
| 153 |
+
|D2⟩ =
|
| 154 |
+
1
|
| 155 |
+
√
|
| 156 |
+
2
|
| 157 |
+
�
|
| 158 |
+
sin2 θ |2−⟩ + cos2 θe−2iϕ |2+⟩ − |2c⟩
|
| 159 |
+
�
|
| 160 |
+
+ 2 sin θ cos θe−iϕ |1+1−⟩ .
|
| 161 |
+
Consequently,
|
| 162 |
+
Aϕ is now a matrix-valued quantity.
|
| 163 |
+
Naively, one might expect that this enables the gener-
|
| 164 |
+
ation of non-Abelian holonomies. However, a direct eval-
|
| 165 |
+
uation of the Eq. (1) leads to
|
| 166 |
+
UA(γ) =
|
| 167 |
+
�
|
| 168 |
+
e2iφ(γ)
|
| 169 |
+
0
|
| 170 |
+
0
|
| 171 |
+
e−2iφ(γ)
|
| 172 |
+
�
|
| 173 |
+
.
|
| 174 |
+
(5)
|
| 175 |
+
It is immediately clear from Eq. (5) that the transforma-
|
| 176 |
+
tions UA(γ) and UA(γ′), induced by two arbitrary loops
|
| 177 |
+
γ and γ′ in M , always commute. Hence, even though de-
|
| 178 |
+
generacy of the system would allow for the generation of
|
| 179 |
+
non-Abelian transformations, the actual holonomy group
|
| 180 |
+
is still Abelian. This phenomenon remains present when
|
| 181 |
+
subjecting even more photons to the system [20], i.e.,
|
| 182 |
+
while degeneracy scales up, the resulting holonomies are
|
| 183 |
+
always commuting.
|
| 184 |
+
The phenomenon that a system’s degeneracy increases
|
| 185 |
+
under the exposure to multiple photons is by no means
|
| 186 |
+
a property unique to the Hamiltonian (3). Adding an
|
| 187 |
+
additional mode to the Λ-scheme leads to a tripod struc-
|
| 188 |
+
ture [Fig. 1 (b)] that allows for any U(2) transforma-
|
| 189 |
+
tion between its single-photon dark states [21–23]. Con-
|
| 190 |
+
sidering two photons, the dark subspace becomes four-
|
| 191 |
+
dimensional. However, as it was noticed in Refs. [14, 24]
|
| 192 |
+
not all elements of the group U(4) can be designed in that
|
| 193 |
+
way (one of the eigenstates decouples). Only, recently
|
| 194 |
+
were these two-particle dynamics verified experimentally
|
| 195 |
+
[15].
|
| 196 |
+
FIG. 1.
|
| 197 |
+
Graph representation of (bilinear) Hamiltonians, in
|
| 198 |
+
which particle number exchange between the modes (vertices)
|
| 199 |
+
is resembled by a connecting edge. (a) Schematic represen-
|
| 200 |
+
tation of three planarly arranged bosonic modes experiencing
|
| 201 |
+
complex next-neighbour coupling κ±. (b) Term scheme of the
|
| 202 |
+
bosonic tripod structure in which the mode c exclusively cou-
|
| 203 |
+
ples to the outer modes µ = ±, 0 via κµ. (c) A four-mode fully
|
| 204 |
+
connected graph, where each side can experience a different
|
| 205 |
+
coupling κµ. (d) Triangular graph of modes with coupling κµ,
|
| 206 |
+
µ = ±, 0.
|
| 207 |
+
B.
|
| 208 |
+
Aim of the article
|
| 209 |
+
This simple introductory example hints at a more gen-
|
| 210 |
+
eral question. What is the number of particles N injected
|
| 211 |
+
into a given setup in order to generate the most versatile
|
| 212 |
+
set of quantum holonomies? After reviewing properties
|
| 213 |
+
of the holonomy group in Sec. II, we address this issue
|
| 214 |
+
by introducing the particle-number threshold (PNT) in
|
| 215 |
+
Sec. III. The PNT of a quantum system gives the min-
|
| 216 |
+
imal number of particles necessary to fully exploit the
|
| 217 |
+
system’s potential for designing non-Abelian holonomies.
|
| 218 |
+
We discuss the basic properties of PNTs and present a
|
| 219 |
+
number of different examples relevant to linear and non-
|
| 220 |
+
|
| 221 |
+
3
|
| 222 |
+
linear quantum optics. Finally, Sec. IV is reserved for
|
| 223 |
+
a summary of the article as well as some concluding re-
|
| 224 |
+
marks.
|
| 225 |
+
II.
|
| 226 |
+
CURVATURE AND UNIVERSALITY
|
| 227 |
+
If the composition of loops in M allows for the genera-
|
| 228 |
+
tion of any unitary on the lth eigenspace Hl of a Hamil-
|
| 229 |
+
tonian ˆH, the connection Al is said to be irreducible, and
|
| 230 |
+
the holonomy group
|
| 231 |
+
Hol(Al) =
|
| 232 |
+
�
|
| 233 |
+
UAl(γ) | γ(0) = γ(T)
|
| 234 |
+
�
|
| 235 |
+
coincides with U(dl). If the eigenspace additionally pos-
|
| 236 |
+
sesses a multi-partite structure (dl = 2k), then Hl may
|
| 237 |
+
be viewed as a k-qubit quantum code [25, 26] on which
|
| 238 |
+
universal manipulation of quantum information is possi-
|
| 239 |
+
ble in terms of holonomic gates UAl(γ) only.
|
| 240 |
+
A convenient measure of how close the group Hol(Al)
|
| 241 |
+
comes to span the entire unitary group, is given in terms
|
| 242 |
+
of the local curvature Fl (the non-Abelian field-strength
|
| 243 |
+
tensor).
|
| 244 |
+
It describes changes of the eigenstates in Hl
|
| 245 |
+
under variation of the parameters κµ. Its antisymmetric
|
| 246 |
+
components (Fl,µν = −Fl,νµ) are calculated from [27]
|
| 247 |
+
Fl,µν = ∂µAl,ν − ∂νAl,µ + [Al,µ, Al,ν].
|
| 248 |
+
(6)
|
| 249 |
+
According to a statement from differential geometry, the
|
| 250 |
+
number of (linear-independent) components {Fl,µν}µν
|
| 251 |
+
gives a lower bound to the dimension of Hol(Al). Here,
|
| 252 |
+
dimension refers to the degrees of freedom that com-
|
| 253 |
+
pletely specify an element in a matrix group. For exam-
|
| 254 |
+
ple, a unitary in U(dl) is completely determined by spec-
|
| 255 |
+
ifying d2
|
| 256 |
+
l real numbers. Hence, we write dim U(dl) = d2
|
| 257 |
+
l .
|
| 258 |
+
This implies, if there are d2
|
| 259 |
+
l linear-independent matrices
|
| 260 |
+
Fl,µν, it is possible to realise any element of the unitary
|
| 261 |
+
group in terms of Eq. (1) [28, 29], i.e., Hol(Al) = U(dl).
|
| 262 |
+
A more accurate bound on the dimension of Hol(Al)
|
| 263 |
+
can be obtained by including higher-order covariant
|
| 264 |
+
derivatives
|
| 265 |
+
∇l,σFl,µν, ∇l,δ∇l,σFl,µν, ∇l,ϵ∇l,δ∇l,σFl,µν, . . . .
|
| 266 |
+
(7)
|
| 267 |
+
Here, the covariant derivative operator
|
| 268 |
+
∇l,σ = ∂σ + [Al,σ, · ]
|
| 269 |
+
generally is different for each eigenspace, thus depending
|
| 270 |
+
on the index l. The number of linearly independent ma-
|
| 271 |
+
trices in Eqs. (6) and (7) equals the dimension of Hol(Al)
|
| 272 |
+
[30, 31].
|
| 273 |
+
Clearly,
|
| 274 |
+
if
|
| 275 |
+
the
|
| 276 |
+
components
|
| 277 |
+
Al,µ
|
| 278 |
+
are
|
| 279 |
+
Abelian,
|
| 280 |
+
then ∇l,σ
|
| 281 |
+
=
|
| 282 |
+
∂σ,
|
| 283 |
+
and the span of the matrices
|
| 284 |
+
{Fl,µν, ∂σFl,µν, . . . }µνσ... is one-dimensional. In follows
|
| 285 |
+
that Hol(Al) is an Abelian subgroup of U(dl).
|
| 286 |
+
Note
|
| 287 |
+
that, even though the above statements do not provide
|
| 288 |
+
an explicit recipe for designing specific transformations,
|
| 289 |
+
there existential nature makes them suitable for estimat-
|
| 290 |
+
ing the general potency of a quantum system to generate
|
| 291 |
+
holonomies. The dimension of the holonomy group acts
|
| 292 |
+
as a natural measure of this potency.
|
| 293 |
+
A.
|
| 294 |
+
Four-mode fully-connected graph
|
| 295 |
+
In order to illustrate the, rather abstract techniques in-
|
| 296 |
+
troduced in the previous section, we give an example of
|
| 297 |
+
a four-mode fully-connected graph, shown in Fig. 1 (c).
|
| 298 |
+
Fully-connected graphs constitute the most general type
|
| 299 |
+
of graphs. Hence, it is not expected that their Hamilto-
|
| 300 |
+
nians possess degenerate eigenvalues when arbitrary con-
|
| 301 |
+
figurations κ = (κµ)µ are considered. Nevertheless, one
|
| 302 |
+
can always construct specific configurations that lead to
|
| 303 |
+
degenerate subspaces. This is done as follows.
|
| 304 |
+
Let ˆH0 be a time-independent Hamiltonian with some
|
| 305 |
+
fixed degeneracy structure.
|
| 306 |
+
Consider the isospectral
|
| 307 |
+
Hamiltonian
|
| 308 |
+
ˆH(κ) = ˆV(κ) ˆH0 ˆV†(κ),
|
| 309 |
+
(8)
|
| 310 |
+
parameterised over points κ = (θ, ϕ) in M . For the four-
|
| 311 |
+
mode system, let ˆH0 = ˆn1 + ˆn2 − ˆn4 (with ˆnk = ˆa†
|
| 312 |
+
kˆak)
|
| 313 |
+
and
|
| 314 |
+
ˆV(θ, ϕ) = ˆV12(θ1, ϕ1) ˆV23(θ2, ϕ2) ˆV34(θ3, ϕ3)
|
| 315 |
+
(9)
|
| 316 |
+
is our unitary of choice. Here, ˆVkk+1(θk, ϕk) creates a
|
| 317 |
+
mixing between the modes k and k+1. More specifically,
|
| 318 |
+
we define
|
| 319 |
+
ˆVkk+1ˆa†
|
| 320 |
+
k ˆV †
|
| 321 |
+
kk+1 = cos θkeiϕkˆa†
|
| 322 |
+
k + sin θkˆa†
|
| 323 |
+
k+1,
|
| 324 |
+
ˆVkk+1ˆa†
|
| 325 |
+
k+1 ˆV †
|
| 326 |
+
kk+1 = cos θke−iϕkˆa†
|
| 327 |
+
k+1 − sin θkˆa†
|
| 328 |
+
k,
|
| 329 |
+
(10)
|
| 330 |
+
which describes a general SU(2) transformation.
|
| 331 |
+
The
|
| 332 |
+
transformation (9) is not the most general unitary, but
|
| 333 |
+
is chosen such that the Hamiltonian (8) is still bilinear
|
| 334 |
+
in the creation and annihilation operators. Thus, it can
|
| 335 |
+
be represented by the graph in Fig. 1 (c).
|
| 336 |
+
If a single particle is subjected to the system, the
|
| 337 |
+
Hamiltonian has a 4 × 4 matrix representation ˆH|F1.
|
| 338 |
+
Here, F1 denotes the first Fock layer, which contains
|
| 339 |
+
the single-particle states |1k⟩ = ˆa†
|
| 340 |
+
k |0⟩. In this Fock layer
|
| 341 |
+
the system has only a single dark state
|
| 342 |
+
|D⟩ = eiϕ3 cos θ3(sin θ1 sin θ2 |11⟩ + e−iϕ1 cos θ1 sin θ2 |12⟩
|
| 343 |
+
+ e−iϕ2 cos θ2 |13⟩) − sin θ3 |14⟩ .
|
| 344 |
+
(11)
|
| 345 |
+
A straight-forward calculation of the corresponding con-
|
| 346 |
+
nection [cf. Eq. (2)] reveals (we omit the index l = 0 for
|
| 347 |
+
notational ease)
|
| 348 |
+
Aϕ1 = −i cos2 θ1 sin2 θ2 cos2 θ3,
|
| 349 |
+
Aϕ2 = −i cos2 θ2 cos2 θ3,
|
| 350 |
+
Aϕ3 = i cos2 θ3,
|
| 351 |
+
and Aθ1 = Aθ2 = Aθ3 = 0.
|
| 352 |
+
The curvature is readily
|
| 353 |
+
calculated from to Eq. (6). Its nonvanishing components
|
| 354 |
+
|
| 355 |
+
4
|
| 356 |
+
are
|
| 357 |
+
Fϕ1θ1 = −2i sin θ1 cos θ1 sin2 θ2 cos2 θ3,
|
| 358 |
+
Fϕ1θ2 = 2i cos2 θ1 sin θ2 cos θ2 cos2 θ3,
|
| 359 |
+
Fϕ1θ3 = −2i cos2 θ1 sin2 θ2 sin θ3 cos θ3,
|
| 360 |
+
Fϕ2θ2 = −2i sin θ2 cos θ2 cos2 θ3,
|
| 361 |
+
Fϕ2θ3 = −2i cos2 θ2 sin θ3 cos θ3,
|
| 362 |
+
Fϕ3θ3 = 2i sin θ3 cos θ3.
|
| 363 |
+
It follows that Abelian holonomies (i.e., Berry phases)
|
| 364 |
+
can be designed by adiabatically traversing loops in M ,
|
| 365 |
+
i.e., Hol(A) = U(1).
|
| 366 |
+
Next, consider the second Fock layer F2 spanned by
|
| 367 |
+
the two-particle states
|
| 368 |
+
|21⟩ , |1112⟩ , |1113⟩ , |1114⟩ , |22⟩ ,
|
| 369 |
+
|1213⟩ , |1214⟩ , |23⟩ , |1314⟩ , |24⟩ .
|
| 370 |
+
The matrix ˆH|F2 supports a three-fold degenerate dark
|
| 371 |
+
subspace with states |Dk⟩, for k = 1, 2, 3 (explicit form
|
| 372 |
+
in Appendix A). The connection on this subspace is
|
| 373 |
+
Aϕ1|θ2=0
|
| 374 |
+
θ1=θ3= π
|
| 375 |
+
4 = i
|
| 376 |
+
2
|
| 377 |
+
�
|
| 378 |
+
�
|
| 379 |
+
0
|
| 380 |
+
0
|
| 381 |
+
0
|
| 382 |
+
0
|
| 383 |
+
1
|
| 384 |
+
ei(ϕ1−ϕ2)
|
| 385 |
+
0 e−i(ϕ1−ϕ2)
|
| 386 |
+
−1
|
| 387 |
+
�
|
| 388 |
+
� ,
|
| 389 |
+
Aϕ2 = i cos2 θ2 cos2 θ3
|
| 390 |
+
�
|
| 391 |
+
�
|
| 392 |
+
−2
|
| 393 |
+
0
|
| 394 |
+
0
|
| 395 |
+
0
|
| 396 |
+
−1 0
|
| 397 |
+
0
|
| 398 |
+
0
|
| 399 |
+
1
|
| 400 |
+
�
|
| 401 |
+
� ,
|
| 402 |
+
Aϕ3 = i cos2 θ3
|
| 403 |
+
�
|
| 404 |
+
�
|
| 405 |
+
2
|
| 406 |
+
0
|
| 407 |
+
0
|
| 408 |
+
0 −1 0
|
| 409 |
+
0
|
| 410 |
+
0
|
| 411 |
+
1
|
| 412 |
+
�
|
| 413 |
+
� ,
|
| 414 |
+
Aθ1 = cos θ2
|
| 415 |
+
�
|
| 416 |
+
�
|
| 417 |
+
0
|
| 418 |
+
0
|
| 419 |
+
0
|
| 420 |
+
0
|
| 421 |
+
0
|
| 422 |
+
−ei(ϕ2−ϕ1)
|
| 423 |
+
0 ei(ϕ2−ϕ1)
|
| 424 |
+
0
|
| 425 |
+
�
|
| 426 |
+
� ,
|
| 427 |
+
and Aθ2 = Aθ3 = 0. Calculating the curvature (6) and its
|
| 428 |
+
first order covariant derivative gives rise to (only linearly
|
| 429 |
+
independent components are shown)
|
| 430 |
+
Fϕ1θ1|κ0 =
|
| 431 |
+
�
|
| 432 |
+
�
|
| 433 |
+
−i
|
| 434 |
+
0
|
| 435 |
+
0
|
| 436 |
+
0
|
| 437 |
+
i
|
| 438 |
+
2
|
| 439 |
+
−
|
| 440 |
+
i
|
| 441 |
+
2
|
| 442 |
+
√
|
| 443 |
+
2
|
| 444 |
+
0
|
| 445 |
+
−
|
| 446 |
+
i
|
| 447 |
+
2
|
| 448 |
+
√
|
| 449 |
+
2
|
| 450 |
+
− i
|
| 451 |
+
2
|
| 452 |
+
�
|
| 453 |
+
� ,
|
| 454 |
+
Fϕ1θ2|κ0 =
|
| 455 |
+
�
|
| 456 |
+
�
|
| 457 |
+
i
|
| 458 |
+
0
|
| 459 |
+
0
|
| 460 |
+
0
|
| 461 |
+
i
|
| 462 |
+
2
|
| 463 |
+
i
|
| 464 |
+
√
|
| 465 |
+
2
|
| 466 |
+
0
|
| 467 |
+
i
|
| 468 |
+
√
|
| 469 |
+
2 − i
|
| 470 |
+
2
|
| 471 |
+
�
|
| 472 |
+
� ,
|
| 473 |
+
Fϕ2θ1|κ0 =
|
| 474 |
+
�
|
| 475 |
+
�
|
| 476 |
+
0 0 0
|
| 477 |
+
0 0 i
|
| 478 |
+
0 i 0
|
| 479 |
+
�
|
| 480 |
+
� ,
|
| 481 |
+
∇ϕ1Fθ1θ2|κ0 =
|
| 482 |
+
�
|
| 483 |
+
�
|
| 484 |
+
0
|
| 485 |
+
0
|
| 486 |
+
0
|
| 487 |
+
0
|
| 488 |
+
i
|
| 489 |
+
−
|
| 490 |
+
i
|
| 491 |
+
2
|
| 492 |
+
√
|
| 493 |
+
2
|
| 494 |
+
0 −
|
| 495 |
+
i
|
| 496 |
+
2
|
| 497 |
+
√
|
| 498 |
+
2
|
| 499 |
+
−i
|
| 500 |
+
�
|
| 501 |
+
� ,
|
| 502 |
+
∇θ1Fϕ2θ1|κ0 =
|
| 503 |
+
�
|
| 504 |
+
�
|
| 505 |
+
0
|
| 506 |
+
0
|
| 507 |
+
0
|
| 508 |
+
0 −i 0
|
| 509 |
+
0
|
| 510 |
+
0
|
| 511 |
+
i
|
| 512 |
+
�
|
| 513 |
+
� ,
|
| 514 |
+
(12)
|
| 515 |
+
evaluated at the point κ0, with ϕk = 0 and θk = π/4.
|
| 516 |
+
The matrices in Eq. (12) are the (infinitesimal) genera-
|
| 517 |
+
tors [32] of a 5-dimensional Lie group. This constitutes
|
| 518 |
+
a lower bound to the dimension of Hol(A). Nevertheless,
|
| 519 |
+
the analysis illustrates that the two-particle case enables
|
| 520 |
+
the generation of more intriguing holonomies than the
|
| 521 |
+
single-particle case. More precisely, the two-particle dark
|
| 522 |
+
states led to a non-Abelian holonomy group Hol(A), that
|
| 523 |
+
is a proper subgroup of U(3).
|
| 524 |
+
The key observation is that, increasing the number of
|
| 525 |
+
particles significantly improved the computational capac-
|
| 526 |
+
ity (from Abelian to non-Abelian holonomies) to gener-
|
| 527 |
+
ate unitaries on the dark subspace. Intuitively, it is clear
|
| 528 |
+
that, the dimension of Hol(A) cannot increase continually
|
| 529 |
+
when the particle number becomes larger, as this would
|
| 530 |
+
result in arbitrarily high computational power, while hav-
|
| 531 |
+
ing only limited physical resources comprised in M . This
|
| 532 |
+
leads us to an interesting question.
|
| 533 |
+
How far can one increase the dimension of the holon-
|
| 534 |
+
omy group by subjecting a larger number of particles to a
|
| 535 |
+
system?
|
| 536 |
+
This question will be addressed in the following section
|
| 537 |
+
by means of a particle-number threshold, which consti-
|
| 538 |
+
tutes a formal answer to the issue.
|
| 539 |
+
III.
|
| 540 |
+
PARTICLE-NUMBER THRESHOLD
|
| 541 |
+
The previously presented benchmark system revealed
|
| 542 |
+
a dependence of a system’s holonomy group on the par-
|
| 543 |
+
ticle number N. Firstly, this is due to the fact that the
|
| 544 |
+
spectral properties (in particular degeneracy) of a quan-
|
| 545 |
+
tum system vary when the corresponding Hamiltonian ˆH
|
| 546 |
+
is limited to act on different Fock layers
|
| 547 |
+
FN =
|
| 548 |
+
�
|
| 549 |
+
|n1, n2 . . .⟩
|
| 550 |
+
���
|
| 551 |
+
�
|
| 552 |
+
k nk = N
|
| 553 |
+
�
|
| 554 |
+
.
|
| 555 |
+
Secondly, we noticed that even if the degeneracy in-
|
| 556 |
+
creases, this does not necessarily mean that it is possible
|
| 557 |
+
to generate a more useful (i.e., higher dimensional) sub-
|
| 558 |
+
group of unitaries.
|
| 559 |
+
Therefore, it is a natural question
|
| 560 |
+
to ask, what is the particle number N at which one of
|
| 561 |
+
the holonomy groups {Hol(Al)}l reaches its maximal di-
|
| 562 |
+
mension and is therefore most suitable for designing a
|
| 563 |
+
versatile set of unitaries. We refer to the number of par-
|
| 564 |
+
ticles necessary for this endeavour as the particle-number
|
| 565 |
+
threshold (PNT) Nt.
|
| 566 |
+
Definition. Let ˆH be the Hamiltonian of a quantum sys-
|
| 567 |
+
tem in second quantisation that evolves adiabatically in
|
| 568 |
+
time. The particle-number threshold Nt denotes the min-
|
| 569 |
+
imum number of particles necessary for one of the sys-
|
| 570 |
+
tem’s holonomy groups to reach its maximum potential
|
| 571 |
+
(maximal dimension) for the generation of holonomies.
|
| 572 |
+
In the language of holonomic quantum computation
|
| 573 |
+
[9, 10] the PNT of a quantum system ˆH gives the number
|
| 574 |
+
of particles to be prepared, in order to come as close
|
| 575 |
+
as possible to the desirable notion of universality.
|
| 576 |
+
In
|
| 577 |
+
|
| 578 |
+
5
|
| 579 |
+
contrast to previous examples, where the focus was on the
|
| 580 |
+
dark subspace, the above definition demands an analysis
|
| 581 |
+
of the holonomy groups of each eigenspace Hl, in order
|
| 582 |
+
to determine dim Hol(Al) for all l. Then, there exists an
|
| 583 |
+
subspace with index l′ such that for all other l
|
| 584 |
+
dim Hol(Al′) ≥ dim Hol(Al)
|
| 585 |
+
holds.
|
| 586 |
+
In other words, the PNT Nt gives the num-
|
| 587 |
+
ber of particles necessary to populate any state in the
|
| 588 |
+
eigenspace Hl′.
|
| 589 |
+
A.
|
| 590 |
+
Properties of PNTs
|
| 591 |
+
The PNT Nt of a (bosonic) quantum system ˆH is, in
|
| 592 |
+
general, hard to calculate, as it demands for a calculation
|
| 593 |
+
of the connection Al for each eigenspace (there could be
|
| 594 |
+
infinitely many). Nevertheless, some general remarks can
|
| 595 |
+
still be made. Consider a quantum system that consists
|
| 596 |
+
of a collection of noninteracting subsystems, i.e., ˆH =
|
| 597 |
+
�
|
| 598 |
+
a ˆHa. Suppose, the PNT N (a)
|
| 599 |
+
t
|
| 600 |
+
for each subsystem ˆHa
|
| 601 |
+
is known and that, Hol
|
| 602 |
+
�
|
| 603 |
+
A(a)
|
| 604 |
+
l′
|
| 605 |
+
�
|
| 606 |
+
denotes its holonomy group
|
| 607 |
+
with maximal dimension. The composite system ˆH then
|
| 608 |
+
has PNT Nt = �
|
| 609 |
+
a N (a)
|
| 610 |
+
t
|
| 611 |
+
.
|
| 612 |
+
This becomes evident when
|
| 613 |
+
noting that the highest-dimensional holonomy group
|
| 614 |
+
Hol(Al′) =
|
| 615 |
+
�
|
| 616 |
+
a
|
| 617 |
+
Hol
|
| 618 |
+
�
|
| 619 |
+
A(a)
|
| 620 |
+
l′
|
| 621 |
+
�
|
| 622 |
+
(13)
|
| 623 |
+
is just the tensor product of the holonomy groups
|
| 624 |
+
Hol
|
| 625 |
+
�
|
| 626 |
+
A(a)
|
| 627 |
+
l′
|
| 628 |
+
�
|
| 629 |
+
of each individual subsystem. The holonomy
|
| 630 |
+
group (13) of the composite system acts on the subspace
|
| 631 |
+
with energy �
|
| 632 |
+
a ε(a)
|
| 633 |
+
l′ , where ε(a)
|
| 634 |
+
l′
|
| 635 |
+
denotes the eigenenergy
|
| 636 |
+
of the subspace on which the group Hol
|
| 637 |
+
�
|
| 638 |
+
A(a)
|
| 639 |
+
l′
|
| 640 |
+
�
|
| 641 |
+
acts.
|
| 642 |
+
Next,
|
| 643 |
+
consider
|
| 644 |
+
a
|
| 645 |
+
Hamiltonian
|
| 646 |
+
with
|
| 647 |
+
isospectral
|
| 648 |
+
parametrisation, that is
|
| 649 |
+
ˆH(κ) = ˆV(κ) ˆH0 ˆV†(κ),
|
| 650 |
+
(14)
|
| 651 |
+
with ˆH0 being a Hamiltonian having fixed degeneracy
|
| 652 |
+
structure {dl}l and eigenstates {|ψl,a⟩}l,a. Suppose there
|
| 653 |
+
is a sufficiently large parameter space M so that ˆV(κ) is
|
| 654 |
+
the most general unitary operator. Adiabatic evolution
|
| 655 |
+
in the lth eigenspace is then governed by the most general
|
| 656 |
+
connection
|
| 657 |
+
(Al,µ)ab = ⟨ψl,b| ˆV†∂µ ˆV |ψl,a⟩ .
|
| 658 |
+
(15)
|
| 659 |
+
In the above, we made use of the fact that ˆV(κ) |ψl,a⟩
|
| 660 |
+
are the eigenstates of (14).
|
| 661 |
+
By construction, one has
|
| 662 |
+
Hol(Al) = U(dl). For such a general parametrisation, it
|
| 663 |
+
is indeed the eigenspace with largest degeneracy dl′ ≥ dl,
|
| 664 |
+
that is the one most desirable for the generation of non-
|
| 665 |
+
Abelian holonomies. Hence, Nt is the number of particles
|
| 666 |
+
necessary to populate any state in the most degenerate
|
| 667 |
+
eigenspace Hl′.
|
| 668 |
+
What happens when ˆV is not an arbitrary unitary,
|
| 669 |
+
but is limited to some smaller set of physically accessi-
|
| 670 |
+
ble operations? For concreteness, consider the two-mode
|
| 671 |
+
Hamiltonian associated with a nonlinear Kerr medium
|
| 672 |
+
ˆH0 = ˆn1(ˆn1 − ˆ1) + ˆn2(ˆn2 − ˆ1).
|
| 673 |
+
Here, the unitary ˆV(α, β, ξ, ζ) is a product of single and
|
| 674 |
+
two-mode displacement
|
| 675 |
+
ˆDk(α) = exp
|
| 676 |
+
�
|
| 677 |
+
αˆa†
|
| 678 |
+
k − α∗ˆak
|
| 679 |
+
�
|
| 680 |
+
,
|
| 681 |
+
ˆK(β) = exp
|
| 682 |
+
�
|
| 683 |
+
βˆa†
|
| 684 |
+
1ˆa2 − β∗ˆa1ˆa†
|
| 685 |
+
2
|
| 686 |
+
�
|
| 687 |
+
,
|
| 688 |
+
(16)
|
| 689 |
+
as well as single and two-mode squeezing
|
| 690 |
+
ˆSk(ξ) = exp
|
| 691 |
+
�
|
| 692 |
+
ξ(ˆa†
|
| 693 |
+
k)2 − ξ∗ˆa2
|
| 694 |
+
k
|
| 695 |
+
�
|
| 696 |
+
,
|
| 697 |
+
ˆ
|
| 698 |
+
M(ζ) = exp
|
| 699 |
+
�
|
| 700 |
+
ζˆa†
|
| 701 |
+
1ˆa†
|
| 702 |
+
2 − ζ∗ˆa1ˆa2
|
| 703 |
+
�
|
| 704 |
+
,
|
| 705 |
+
(17)
|
| 706 |
+
respectively [33].
|
| 707 |
+
By driving coherent displacement
|
| 708 |
+
(α, β) and squeezing parameters (ξ, ζ) through a closed
|
| 709 |
+
loop in M = C4, holonomies on the eigenspaces of ˆH
|
| 710 |
+
are obtained. In Ref. [34] it was shown that this enables
|
| 711 |
+
arbitrary U(4) transformations over the zero-eigenvalue
|
| 712 |
+
eigenspace H0. The subspace is spanned by the number
|
| 713 |
+
states |0102⟩, |1102⟩, |0112⟩, and |1112⟩, i.e., two photons
|
| 714 |
+
are necessary to fully occupy the subspace.
|
| 715 |
+
An extended study (up to N = 50) of the curvature
|
| 716 |
+
Fl shows that, even though further increasing the parti-
|
| 717 |
+
cle number (N > 2) populates subspaces with increased
|
| 718 |
+
degeneracy (up to dl = 10 for some eigenspaces), their
|
| 719 |
+
holonomy groups do not offer a computational advantage.
|
| 720 |
+
By that we mean
|
| 721 |
+
dim Hol(Al) ≤ dim Hol(A0)
|
| 722 |
+
verified for all eigenspaces Hl with index l ≤ 352 (cf.
|
| 723 |
+
Tab. I). We did so by explicitly calculating the compo-
|
| 724 |
+
nents Fl,µν of the curvature and their covariant deriva-
|
| 725 |
+
tives up to order 3, (these are to large to be displayed
|
| 726 |
+
here). The computed dimension of the groups {Hol(Al)}l
|
| 727 |
+
did not increase further after the first order derivatives,
|
| 728 |
+
thus giving us good confidence that the dimension was
|
| 729 |
+
determined accurately.
|
| 730 |
+
There is an intuitive explanation for the fact that
|
| 731 |
+
eigenspaces involving higher particle numbers (N > 6)
|
| 732 |
+
lead to less useful holonomy groups. The Gaussian op-
|
| 733 |
+
erations (16) and (17) contribute to the evolution only
|
| 734 |
+
via the connection Al.
|
| 735 |
+
The derivative ∂µ in Eq.
|
| 736 |
+
(15)
|
| 737 |
+
that acts on the operators (16) and (17), leads to cre-
|
| 738 |
+
ation and annihilation operators of (at most) quadratic
|
| 739 |
+
order. Hence, Fock states with larger differences in their
|
| 740 |
+
photon numbers cannot be transformed into each other
|
| 741 |
+
by a quantum holonomy, even when they lie in the same
|
| 742 |
+
subspace.
|
| 743 |
+
In summary, the subspace H0 (containing at most two-
|
| 744 |
+
particle states) should be preferred when the system is
|
| 745 |
+
utilised in a holonomic quantum computation.
|
| 746 |
+
There-
|
| 747 |
+
fore, the PNT of the two-mode Kerr Hamiltonian is
|
| 748 |
+
|
| 749 |
+
6
|
| 750 |
+
Nt = 2.
|
| 751 |
+
Moreover, it was shown that restricting the
|
| 752 |
+
parametrisation of the Hamiltonian (14) to unitaries ˆV
|
| 753 |
+
that can be implemented by Gaussian operations (16)
|
| 754 |
+
and (17), led to most of the system’s eigenspaces hav-
|
| 755 |
+
ing reducible connections Al, i.e., Hol(Al) ⊂ U(dl).
|
| 756 |
+
Hence, degeneracy became a quantity of secondary in-
|
| 757 |
+
terest. In Tab. I the spectral properties of the two-mode
|
| 758 |
+
Kerr Hamiltonian ˆH are listed together with their ca-
|
| 759 |
+
pacity to generate holonomies on the eigenspaces Hl (for
|
| 760 |
+
l = 0, . . . , 352).
|
| 761 |
+
Note that subspaces with degeneracy
|
| 762 |
+
dl ≤ 4 are not listed in in Tab. I, as it is already clear
|
| 763 |
+
that their holonomy groups cannot exceed the dimension
|
| 764 |
+
of Hol(A0) = U(4).
|
| 765 |
+
B.
|
| 766 |
+
PNTs of coupled harmonic oscillators
|
| 767 |
+
While the exact calculation of a PNT can be a daunting
|
| 768 |
+
task, given a collection of coupled harmonic oscillators,
|
| 769 |
+
certain specialisations arise that can simplify calculations
|
| 770 |
+
drastically. In Fig. 1 such systems were represented as
|
| 771 |
+
graphs. The calculation of PNTs for such systems would
|
| 772 |
+
be relevant, for instance, to the geometric manipulation
|
| 773 |
+
of multi-photon states in linear optics [14] as well as linear
|
| 774 |
+
optical quantum computation by holonomic means [20].
|
| 775 |
+
Population transfer between different Fock layers FN
|
| 776 |
+
does not occur in these systems, as the total number of
|
| 777 |
+
particles stays conserved throughout an evolution. From
|
| 778 |
+
a mathematical viewpoint, this implies that the system’s
|
| 779 |
+
Hamiltonian reveals a block-matrix structure, i.e.,
|
| 780 |
+
ˆH =
|
| 781 |
+
�
|
| 782 |
+
N∈N
|
| 783 |
+
ˆH|FN .
|
| 784 |
+
In addition, there always exists a spectral decomposition
|
| 785 |
+
ˆH = �
|
| 786 |
+
l εl ˆΠl, with ˆΠl denoting the projector onto the
|
| 787 |
+
eigenspace Hl. It follows that the eigenspaces themselves
|
| 788 |
+
admit a similar decomposition, that is
|
| 789 |
+
ˆΠl =
|
| 790 |
+
�
|
| 791 |
+
N(l)
|
| 792 |
+
ˆΠl|FN(l),
|
| 793 |
+
(18)
|
| 794 |
+
where summation is carried out over those particle num-
|
| 795 |
+
bers N(l) at which the corresponding energy εl occurs.
|
| 796 |
+
As an example, the Hamiltonian (3) of the Λ-scheme
|
| 797 |
+
[Fig. 1. (a)] does not possess single-particle eigenstates
|
| 798 |
+
with energy 2
|
| 799 |
+
�
|
| 800 |
+
|κ+|2 + |κ−|2. In other words the eigen-
|
| 801 |
+
value does not lie in the spectrum of ˆH|F1, but it is an
|
| 802 |
+
eigenvalue of the matrix ˆH|FN for N ≥ 2. In this case,
|
| 803 |
+
the sum in Eq.
|
| 804 |
+
(18) corresponds to an infinite series
|
| 805 |
+
starting with N(l) = 2, 3, . . . .
|
| 806 |
+
If additionally the evolution is assumed to be adia-
|
| 807 |
+
batic, population transfer occurs within each eigenspace
|
| 808 |
+
separately. Hence, the decomposition (18) is inherited to
|
| 809 |
+
the time-evolution operator (quantum holonomy)
|
| 810 |
+
UAl(γ) =
|
| 811 |
+
�
|
| 812 |
+
N(l)
|
| 813 |
+
UAl(γ)|FN(l).
|
| 814 |
+
(19)
|
| 815 |
+
l
|
| 816 |
+
εl
|
| 817 |
+
dl
|
| 818 |
+
≤ N
|
| 819 |
+
dim{Fl,µν}µν dim Hol(Al)
|
| 820 |
+
0
|
| 821 |
+
0
|
| 822 |
+
4
|
| 823 |
+
2
|
| 824 |
+
14
|
| 825 |
+
16
|
| 826 |
+
1
|
| 827 |
+
2
|
| 828 |
+
4
|
| 829 |
+
3
|
| 830 |
+
14
|
| 831 |
+
16
|
| 832 |
+
5
|
| 833 |
+
12
|
| 834 |
+
5
|
| 835 |
+
6
|
| 836 |
+
9
|
| 837 |
+
9
|
| 838 |
+
16
|
| 839 |
+
42
|
| 840 |
+
6
|
| 841 |
+
10
|
| 842 |
+
9
|
| 843 |
+
9
|
| 844 |
+
26
|
| 845 |
+
72
|
| 846 |
+
6
|
| 847 |
+
13
|
| 848 |
+
12
|
| 849 |
+
12
|
| 850 |
+
37
|
| 851 |
+
110
|
| 852 |
+
6
|
| 853 |
+
15
|
| 854 |
+
9
|
| 855 |
+
9
|
| 856 |
+
45
|
| 857 |
+
132
|
| 858 |
+
6
|
| 859 |
+
17
|
| 860 |
+
9
|
| 861 |
+
9
|
| 862 |
+
54
|
| 863 |
+
162
|
| 864 |
+
6
|
| 865 |
+
19
|
| 866 |
+
6
|
| 867 |
+
6
|
| 868 |
+
60
|
| 869 |
+
182
|
| 870 |
+
6
|
| 871 |
+
20
|
| 872 |
+
9
|
| 873 |
+
9
|
| 874 |
+
70
|
| 875 |
+
212
|
| 876 |
+
6
|
| 877 |
+
21
|
| 878 |
+
3
|
| 879 |
+
3
|
| 880 |
+
78
|
| 881 |
+
240
|
| 882 |
+
6
|
| 883 |
+
21
|
| 884 |
+
9
|
| 885 |
+
9
|
| 886 |
+
87
|
| 887 |
+
272
|
| 888 |
+
6
|
| 889 |
+
24
|
| 890 |
+
9
|
| 891 |
+
9
|
| 892 |
+
99
|
| 893 |
+
312
|
| 894 |
+
5
|
| 895 |
+
26
|
| 896 |
+
3
|
| 897 |
+
3
|
| 898 |
+
108
|
| 899 |
+
342
|
| 900 |
+
6
|
| 901 |
+
27
|
| 902 |
+
9
|
| 903 |
+
9
|
| 904 |
+
113
|
| 905 |
+
362
|
| 906 |
+
6
|
| 907 |
+
27
|
| 908 |
+
3
|
| 909 |
+
3
|
| 910 |
+
130
|
| 911 |
+
420
|
| 912 |
+
5
|
| 913 |
+
30
|
| 914 |
+
9
|
| 915 |
+
9
|
| 916 |
+
131
|
| 917 |
+
422
|
| 918 |
+
6
|
| 919 |
+
30
|
| 920 |
+
3
|
| 921 |
+
3
|
| 922 |
+
141
|
| 923 |
+
462
|
| 924 |
+
8
|
| 925 |
+
31
|
| 926 |
+
9
|
| 927 |
+
9
|
| 928 |
+
157
|
| 929 |
+
512
|
| 930 |
+
6
|
| 931 |
+
33
|
| 932 |
+
6
|
| 933 |
+
6
|
| 934 |
+
168
|
| 935 |
+
552
|
| 936 |
+
10
|
| 937 |
+
34
|
| 938 |
+
9
|
| 939 |
+
9
|
| 940 |
+
199
|
| 941 |
+
662
|
| 942 |
+
6
|
| 943 |
+
36
|
| 944 |
+
3
|
| 945 |
+
3
|
| 946 |
+
208
|
| 947 |
+
702
|
| 948 |
+
6
|
| 949 |
+
38
|
| 950 |
+
9
|
| 951 |
+
9
|
| 952 |
+
215
|
| 953 |
+
722
|
| 954 |
+
6
|
| 955 |
+
39
|
| 956 |
+
6
|
| 957 |
+
6
|
| 958 |
+
222
|
| 959 |
+
756
|
| 960 |
+
6
|
| 961 |
+
38
|
| 962 |
+
9
|
| 963 |
+
9
|
| 964 |
+
225
|
| 965 |
+
762
|
| 966 |
+
6
|
| 967 |
+
40
|
| 968 |
+
3
|
| 969 |
+
3
|
| 970 |
+
238
|
| 971 |
+
812
|
| 972 |
+
10
|
| 973 |
+
41
|
| 974 |
+
9
|
| 975 |
+
9
|
| 976 |
+
266
|
| 977 |
+
912
|
| 978 |
+
6
|
| 979 |
+
42
|
| 980 |
+
3
|
| 981 |
+
3
|
| 982 |
+
274
|
| 983 |
+
942
|
| 984 |
+
8
|
| 985 |
+
44
|
| 986 |
+
3
|
| 987 |
+
3
|
| 988 |
+
285
|
| 989 |
+
992
|
| 990 |
+
6
|
| 991 |
+
45
|
| 992 |
+
9
|
| 993 |
+
9
|
| 994 |
+
306
|
| 995 |
+
1062
|
| 996 |
+
8
|
| 997 |
+
47
|
| 998 |
+
3
|
| 999 |
+
3
|
| 1000 |
+
320
|
| 1001 |
+
1112
|
| 1002 |
+
6
|
| 1003 |
+
48
|
| 1004 |
+
3
|
| 1005 |
+
3
|
| 1006 |
+
323
|
| 1007 |
+
1122
|
| 1008 |
+
6
|
| 1009 |
+
48
|
| 1010 |
+
9
|
| 1011 |
+
9
|
| 1012 |
+
346
|
| 1013 |
+
1202
|
| 1014 |
+
8
|
| 1015 |
+
50
|
| 1016 |
+
3
|
| 1017 |
+
3
|
| 1018 |
+
349
|
| 1019 |
+
1212
|
| 1020 |
+
6
|
| 1021 |
+
49
|
| 1022 |
+
3
|
| 1023 |
+
3
|
| 1024 |
+
352
|
| 1025 |
+
1232
|
| 1026 |
+
8
|
| 1027 |
+
50
|
| 1028 |
+
3
|
| 1029 |
+
3
|
| 1030 |
+
TABLE I.
|
| 1031 |
+
Holonomy groups of the two-mode nonlinear
|
| 1032 |
+
Kerr medium parameterised by the Gaussian operations (16)
|
| 1033 |
+
and (17).
|
| 1034 |
+
The table contains the degeneracy dl of the lth
|
| 1035 |
+
eigenspace (with energy εl). N denotes the number of parti-
|
| 1036 |
+
cles necessary to fully occupy the corresponding eigenspace.
|
| 1037 |
+
The number of linear-independent curvature components
|
| 1038 |
+
Fl,µν as well as the dimension of the holonomy group Hol(Al).
|
| 1039 |
+
Covariant derivatives were calculated up the order of 3.
|
| 1040 |
+
Remarkably, the connection will always be reducible for
|
| 1041 |
+
such a system, because it is not possible to generate
|
| 1042 |
+
transformations between different Fock layers. The best
|
| 1043 |
+
one can hope for, is to find is a highly-degenerate N-
|
| 1044 |
+
particle block in the eigenspace Hl such that the holon-
|
| 1045 |
+
omy UAl(γ)|FN realises any unitary transformation on
|
| 1046 |
+
the subspace Hl|FN .
|
| 1047 |
+
This is nothing but a geometric
|
| 1048 |
+
|
| 1049 |
+
7
|
| 1050 |
+
incarnation of the well-known fact that networks of cou-
|
| 1051 |
+
pled oscillators (by themselves) do not allow for univer-
|
| 1052 |
+
sal quantum computation [35], but must be supported by
|
| 1053 |
+
additional resources, such as measurement-induced non-
|
| 1054 |
+
linearities [36, 37].
|
| 1055 |
+
Note that, even though the quantum holonomy (19)
|
| 1056 |
+
can have an infinite-dimensional matrix representation,
|
| 1057 |
+
it might still be commuting, that is UAl(γ)UAl(γ′) =
|
| 1058 |
+
UAl(γ′)UAl(γ) for any two loops γ and γ′ in M .
|
| 1059 |
+
For
|
| 1060 |
+
the purpose of illustration, consider the Hamiltonian (3)
|
| 1061 |
+
of the Λ-scheme [cf. Fig. 1 (a)] which gives rise to an
|
| 1062 |
+
infinite-dimensional dark subspace. For a single photon,
|
| 1063 |
+
the matrix ˆH|F1 has only one dark state. Given two or
|
| 1064 |
+
three photons in the setup, ˆH|F2 and ˆH|F3 both have
|
| 1065 |
+
two dark states. Subjecting four photons to the system
|
| 1066 |
+
leads to a Hamiltonian matrix ˆH|F4 having three dark
|
| 1067 |
+
states.
|
| 1068 |
+
Even though degeneracy further increases, the
|
| 1069 |
+
quantum holonomy
|
| 1070 |
+
UA0 =
|
| 1071 |
+
�
|
| 1072 |
+
��
|
| 1073 |
+
UA0|F1
|
| 1074 |
+
UA0|F2
|
| 1075 |
+
...
|
| 1076 |
+
�
|
| 1077 |
+
��
|
| 1078 |
+
will remain Abelian, because the N-particle block
|
| 1079 |
+
UA0(γ)|FN = diag
|
| 1080 |
+
�
|
| 1081 |
+
eiNφ(γ), e−iNφ(γ), eiNφ(γ), . . .
|
| 1082 |
+
�
|
| 1083 |
+
,
|
| 1084 |
+
is itself a diagonal matrix [cf. Eq. (5) for N = 2]. Here,
|
| 1085 |
+
φ(γ) is the geometric phase defined in Eq. (4). The above
|
| 1086 |
+
analysis illustrates, that increasing the particle number in
|
| 1087 |
+
the photonic Λ-scheme does not increase the holonomy
|
| 1088 |
+
group’s dimension, i.e., it stays Abelian. Similar argu-
|
| 1089 |
+
ments hold for the other eigenspaces of the system, and
|
| 1090 |
+
thus a single photon is sufficient to generate any phase
|
| 1091 |
+
in U(1). Hence, the PNT is Nt = 1.
|
| 1092 |
+
1.
|
| 1093 |
+
Three-mode fully-connected graph
|
| 1094 |
+
Consider a setup containing three oscillator modes ˆa±
|
| 1095 |
+
and ˆa0. Coupling between the modes is described by the
|
| 1096 |
+
parameters κ± and κ0, respectively. The system corre-
|
| 1097 |
+
sponds to the three-mode fully-connected graph shown
|
| 1098 |
+
in Fig. 1 (d).
|
| 1099 |
+
For simplicity, its Hamiltonian is considered to be in
|
| 1100 |
+
the configuration
|
| 1101 |
+
ˆH(θ, ϕ) = ˆV(θ, ϕ) ˆH0 ˆV†(θ, ϕ),
|
| 1102 |
+
(20)
|
| 1103 |
+
with ˆH0 = ˆn+ − ˆn−. In the above,
|
| 1104 |
+
ˆV(θ, ϕ) = ˆV+0(θ+, ϕ+) ˆV0−(��−, ϕ−),
|
| 1105 |
+
with the operator ˆVkk+1 defined in Eq. (10). The 3 × 3
|
| 1106 |
+
matrix ˆH|F1 possesses single-particle eigenstates
|
| 1107 |
+
|B+⟩ = cos θ+eiϕ+ |1+⟩ − sin θ− |10⟩ ,
|
| 1108 |
+
|D⟩ = cos θ−eiϕ−�
|
| 1109 |
+
cos θ+e−iϕ+ |1+⟩ − sin θ+ |10⟩
|
| 1110 |
+
�
|
| 1111 |
+
− sin θ− |1−⟩ ,
|
| 1112 |
+
|B−⟩ = cos θ−e−iϕ− |1−⟩
|
| 1113 |
+
− sin θ−
|
| 1114 |
+
�
|
| 1115 |
+
cos θ+e−iϕ+ |10⟩ − sin θ+ |1+⟩
|
| 1116 |
+
�
|
| 1117 |
+
,
|
| 1118 |
+
with eigenenergies ε± = ±1 and ε0 = 0. The connec-
|
| 1119 |
+
tion for each eigenvalue is readily calculated via Eq. (2),
|
| 1120 |
+
leading to the nonvanishing components
|
| 1121 |
+
A+,ϕ+ = i cos2 θ+,
|
| 1122 |
+
A0,ϕ± = i cos2 θ±,
|
| 1123 |
+
A−,ϕ+ = −i sin2 θ+ cos2 θ+,
|
| 1124 |
+
A−,ϕ− = −i cos2 θ−.
|
| 1125 |
+
When given more than just a single particle, the Hamil-
|
| 1126 |
+
tonian (20) gives rise to degenerate subspaces, e.g., con-
|
| 1127 |
+
sidering two-particles in the system, the 6 × 6 matrix
|
| 1128 |
+
ˆH|F2 possesses two dark states. However, in the follow-
|
| 1129 |
+
ing it will be shown that the resulting holonomies are
|
| 1130 |
+
still Abelian for arbitrary particle numbers N. It is a
|
| 1131 |
+
well known fact for coupled-mode systems, that knowing
|
| 1132 |
+
the single-particle evolution is equivalent to knowing the
|
| 1133 |
+
evolution of the modes ˆak(t) in the Heisenberg picture
|
| 1134 |
+
[33], viz.
|
| 1135 |
+
ˆa†
|
| 1136 |
+
±(T) = e∓iT e
|
| 1137 |
+
¸
|
| 1138 |
+
A±ˆa†
|
| 1139 |
+
±(0),
|
| 1140 |
+
ˆa†
|
| 1141 |
+
0(T) = e
|
| 1142 |
+
¸
|
| 1143 |
+
A0ˆa†
|
| 1144 |
+
0(0).
|
| 1145 |
+
Subsequently, the evolution of any N-particle state can
|
| 1146 |
+
be given explicitly. It follows the state can only attain a
|
| 1147 |
+
Berry phase as well. The initial N-particle state
|
| 1148 |
+
|Ψ(0)⟩ =
|
| 1149 |
+
1
|
| 1150 |
+
�
|
| 1151 |
+
n+!n0!n−!
|
| 1152 |
+
�
|
| 1153 |
+
ˆa†
|
| 1154 |
+
+
|
| 1155 |
+
�n+�
|
| 1156 |
+
ˆa†
|
| 1157 |
+
0
|
| 1158 |
+
�n0�
|
| 1159 |
+
ˆa†
|
| 1160 |
+
−
|
| 1161 |
+
�n− |0⟩
|
| 1162 |
+
(N = n+ + n0 + n−) adiabatically evolves into
|
| 1163 |
+
|Ψ(T)⟩ = en+
|
| 1164 |
+
¸
|
| 1165 |
+
A+en0
|
| 1166 |
+
¸
|
| 1167 |
+
A0en−
|
| 1168 |
+
¸
|
| 1169 |
+
A− |n+⟩ ⊗ |n0⟩ ⊗ |n−⟩ ,
|
| 1170 |
+
accumulating a (scalar) geometric phase.
|
| 1171 |
+
We this conclude that, independent of the provided
|
| 1172 |
+
particle number N, the holonomy group can only be
|
| 1173 |
+
Abelian.
|
| 1174 |
+
Hence, the PNT of the system is Nt = 1,
|
| 1175 |
+
as moving beyond the single-particle case did not lead
|
| 1176 |
+
to more versatile groups of holonomies but just higher-
|
| 1177 |
+
dimensional representations of the group U(1).
|
| 1178 |
+
The
|
| 1179 |
+
above argument is the special case of a more general
|
| 1180 |
+
bosonic-operator framework, which we devised in Ref.
|
| 1181 |
+
[20]. This formalism enables a photon-number indepen-
|
| 1182 |
+
dent description of holonomies, and thus might be useful
|
| 1183 |
+
for the calculation of PNTs in coupled-mode systems.
|
| 1184 |
+
C.
|
| 1185 |
+
PNTs of fermionic systems
|
| 1186 |
+
So far, all considered quantum systems were bosonic
|
| 1187 |
+
in nature. Nevertheless, the definition of a PNT is appli-
|
| 1188 |
+
cable to any quantum system given in second quantisa-
|
| 1189 |
+
tion (cf. Sec. III). Fermionic modes are associated with
|
| 1190 |
+
|
| 1191 |
+
8
|
| 1192 |
+
creation and annihilation operators satisfying canonical
|
| 1193 |
+
anticommutation relations.
|
| 1194 |
+
Because of this, the most
|
| 1195 |
+
prominent difference to the bosonic setups studied previ-
|
| 1196 |
+
ously, is that fermions have to obey the Pauli principle,
|
| 1197 |
+
i.e., two fermions cannot occupy the same mode simulta-
|
| 1198 |
+
neously. This drastically reduces the number of possible
|
| 1199 |
+
states in a system and in particular, the corresponding
|
| 1200 |
+
Hilbert space (Fock space) is finite dimensional. Hence,
|
| 1201 |
+
the calculation of the PNT of a fermionic system be-
|
| 1202 |
+
comes much more manageable in comparison to bosonic
|
| 1203 |
+
systems.
|
| 1204 |
+
PNTs can also be calculated for systems comprising
|
| 1205 |
+
both bosonic and fermionic modes. As an elementary ex-
|
| 1206 |
+
ample, consider the Jaynes-Cummings Hamiltonian de-
|
| 1207 |
+
scribing the interaction between an incident light field
|
| 1208 |
+
and a single atomic energy level at resonance. Within
|
| 1209 |
+
the rotating wave approximation, the Hamiltonian reads
|
| 1210 |
+
[33]
|
| 1211 |
+
ˆHJC = ωAˆσ+ˆσ− + ωcˆn + κ
|
| 1212 |
+
�
|
| 1213 |
+
ˆa†ˆσ− + ˆaˆσ+�
|
| 1214 |
+
,
|
| 1215 |
+
with resonance frequency ωA of the atom, ωc being the
|
| 1216 |
+
frequency of the incident light field, and κ describing the
|
| 1217 |
+
strength of the light-matter interaction. The atomic lad-
|
| 1218 |
+
der operators ˆσ− and ˆσ+ = (ˆσ−)† shift an electron from
|
| 1219 |
+
the ground to the excited state, and vice versa. The sys-
|
| 1220 |
+
tem possesses a nondegenerate spectrum {εn±}n∈N with
|
| 1221 |
+
corresponding eigenstates
|
| 1222 |
+
|n+⟩ = sin θ |g, n + 1⟩ + cos θ |e, n⟩ ,
|
| 1223 |
+
|n−⟩ = cos θ |g, n + 1⟩ − sin θ |e, n⟩ ,
|
| 1224 |
+
where tan(2θ) = 2κ√n + 1/(ωc − ωA) and n being the
|
| 1225 |
+
photon number. This form of the eigenstates highlights
|
| 1226 |
+
that the underlying parameter space does not possess any
|
| 1227 |
+
curvature, i.e., Fn±,θθ = 0 for all photon numbers n ∈ N.
|
| 1228 |
+
Hence, the system is not suitable for the generation of
|
| 1229 |
+
quantum holonomies, and this is reflected in the PNT,
|
| 1230 |
+
i.e., Nt = 0.
|
| 1231 |
+
IV.
|
| 1232 |
+
DISCUSSION
|
| 1233 |
+
In this article we studied quantum holonomies in rela-
|
| 1234 |
+
tion to the particle number in a system. It was shown
|
| 1235 |
+
that, increasing the number of particles can lead to a
|
| 1236 |
+
higher-dimensional holonomy group, thus improving the
|
| 1237 |
+
capabilities of the system to generate useful unitaries.
|
| 1238 |
+
We introduced the PNT of a quantum system, which de-
|
| 1239 |
+
notes the minimal number of particles necessary to fully
|
| 1240 |
+
exploit the systems capacity for generating a versatile set
|
| 1241 |
+
of quantum holonomies. Besides some general statements
|
| 1242 |
+
that could be made about PNTs, we illustrated the the-
|
| 1243 |
+
ory in terms of benchmark examples relevant to linear
|
| 1244 |
+
and nonlinear quantum optics. We saw that for systems
|
| 1245 |
+
of coupled oscillators only the Nt-particle block of an
|
| 1246 |
+
eigenspace contributes to its holonomy group relevantly,
|
| 1247 |
+
because the particle number Nt subjected to the system
|
| 1248 |
+
does not change throughout the propagation. This result
|
| 1249 |
+
appears to be relevant to linear optical quantum compu-
|
| 1250 |
+
tation by adiabatic means. We argued that the results
|
| 1251 |
+
presented are applicable to both bosonic and fermionic
|
| 1252 |
+
systems of interest. Our general investigation hints at the
|
| 1253 |
+
utility of the concept in assessing the capabilities of dif-
|
| 1254 |
+
ferent quantum systems to perform holonomic quantum
|
| 1255 |
+
computations in terms of holonomies. PNTs might also
|
| 1256 |
+
be relevant to the simulation of gauge groups in terms of
|
| 1257 |
+
adiabatic parameter variations.
|
| 1258 |
+
Currently, there is a lack of analytical tools to compute
|
| 1259 |
+
PNTs. While this is a straight forward task for fermionic
|
| 1260 |
+
systems, it becomes a challenging issue for bosonic sys-
|
| 1261 |
+
tems, where there is no bound on the particle number.
|
| 1262 |
+
Estimations of the PNT up to some finite particle num-
|
| 1263 |
+
ber, might be sufficient for most practical purposes, but
|
| 1264 |
+
general strategies for calculating PNTs can be relevant
|
| 1265 |
+
for a deeper understanding of many-particle physics in
|
| 1266 |
+
an adiabatic setting.
|
| 1267 |
+
ACKNOWLEDGMENTS
|
| 1268 |
+
Financial support by the Deutsche Forschungsgemein-
|
| 1269 |
+
schaft (DFG SCHE 612/6-1) is gratefully acknowledged.
|
| 1270 |
+
Appendix A: Two-particle dark states of the
|
| 1271 |
+
four-mode fully-connected graph
|
| 1272 |
+
In this appendix, we give the two-particle dark states
|
| 1273 |
+
of the Hamiltonian matrix ˆH|F2 of the four-mode fully-
|
| 1274 |
+
connected graph shown in Fig. 1 (c). The isospectral
|
| 1275 |
+
Hamiltonian of the system is given in Eq. (8). The three
|
| 1276 |
+
dark states of the system read
|
| 1277 |
+
|D1⟩ =
|
| 1278 |
+
1
|
| 1279 |
+
√
|
| 1280 |
+
2
|
| 1281 |
+
�
|
| 1282 |
+
eiϕ3 sin θ1 sin θ2 cos θ3ˆa†
|
| 1283 |
+
1 + ei(ϕ3−ϕ1) cos θ1 sin θ2 cos θ3ˆa†
|
| 1284 |
+
2 + ei(ϕ3−ϕ2) cos θ2 cos θ3ˆa†
|
| 1285 |
+
3 − sin θ3ˆa†
|
| 1286 |
+
4
|
| 1287 |
+
�2 |0⟩ ,
|
| 1288 |
+
|D2⟩ =
|
| 1289 |
+
�
|
| 1290 |
+
sin θ1 sin θ2 sin θ3ˆa†
|
| 1291 |
+
1 + e−iϕ1 cos θ1 sin θ2 sin θ3ˆa†
|
| 1292 |
+
2 + e−iϕ2 cos θ2 sin θ3ˆa†
|
| 1293 |
+
3 + e−iϕ3 cos θ3ˆa†
|
| 1294 |
+
4
|
| 1295 |
+
�
|
| 1296 |
+
×
|
| 1297 |
+
�
|
| 1298 |
+
eiϕ1 cos θ1ˆa†
|
| 1299 |
+
1 − sin θ1ˆa†
|
| 1300 |
+
2
|
| 1301 |
+
�
|
| 1302 |
+
|0⟩ ,
|
| 1303 |
+
|D3⟩ =
|
| 1304 |
+
�
|
| 1305 |
+
sin θ1 sin θ2 sin θ3ˆa†
|
| 1306 |
+
1 + e−iϕ1 cos θ1 sin θ2 sin θ3ˆa†
|
| 1307 |
+
2 + e−iϕ2 cos θ2 sin θ3ˆa†
|
| 1308 |
+
3 + e−iϕ3 cos θ3ˆa†
|
| 1309 |
+
4
|
| 1310 |
+
�
|
| 1311 |
+
×
|
| 1312 |
+
�
|
| 1313 |
+
eiϕ1 sin θ1 cos θ2ˆa†
|
| 1314 |
+
1 + ei(ϕ2−ϕ1) cos θ1 cos θ2ˆa†
|
| 1315 |
+
2
|
| 1316 |
+
�
|
| 1317 |
+
|0⟩ ,
|
| 1318 |
+
|
| 1319 |
+
9
|
| 1320 |
+
where the parameter angles (θk, ϕk) are defined in Eq. (10).
|
| 1321 |
+
[1] M. V. Berry, Quantal Phase Factors Accompanying Adi-
|
| 1322 |
+
abatic Changes, Proc. R. Soc. London, Ser. A 392, 45
|
| 1323 |
+
(1984).
|
| 1324 |
+
[2] Y. Aharonov and D. Bohm, Significance of Electromag-
|
| 1325 |
+
netic Potentials in the Quantum Theory, Phys. Rev. 115,
|
| 1326 |
+
485 (1959).
|
| 1327 |
+
[3] S. Pancharatnam, Generalized theory of interference, and
|
| 1328 |
+
its applications, Proc.-Indian Acad. Sci. Sect. A. 44, 247
|
| 1329 |
+
(1956).
|
| 1330 |
+
[4] B. Simon, Holonomy, the Quantum Adiabatic Theorem,
|
| 1331 |
+
and Berry’s Phase, Phys. Rev. Lett. 51, 2167 (1983).
|
| 1332 |
+
[5] M. Born and V. A. Fock, Beweis des Adiabatensatzes, Z.
|
| 1333 |
+
Phys. 51, 165 (1928).
|
| 1334 |
+
[6] F. Wilczek and A. Zee, Appearance of Gauge Structure
|
| 1335 |
+
in Simple Dynamical Systems, Phys. Rev. Lett. 52, 2111
|
| 1336 |
+
(1984).
|
| 1337 |
+
[7] M. C. Ba˜nuls and K. Cichy, Review on novel methods
|
| 1338 |
+
for lattice gauge theories, Rep. Prog. Phys. 83, 024401
|
| 1339 |
+
(2020).
|
| 1340 |
+
[8] C. Rovelli, Loop Quantum Gravity, Living Rev. Relativ.
|
| 1341 |
+
11, 5 (2008).
|
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