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33eb6fff4beeb69658f6f438af46e2d0014f0672
subsection
13
40
Comparison with the cyclic module of the algebra
Let \mathsf {H} be a cocommutative Hopf algebra. In this section, we construct an injective cyclic module map \tau :\mathrm {B}(\mathsf {H})\rightarrow C(\mathsf {H}), from the cyclic bar complex \mathrm {B}(\mathsf {H}) of REF to the canonical cyclic k-module C(\mathsf {H}) of the algebra underlying \mathsf {H} (), an...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 403, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
[ 10842, 125458, 420, 841, 186, 552, 277, 68754, 5844, 101082, 144, 429, 2844, 903, 40059, 64549, 115049, 187830, 238, 88996, 22288, 50104, 571, 54969, 313, 1295, 1909, 27140, 9069, 919, 74413, 472, 83279, 1379, 60520, 501, 47, 40907, 79059, ...
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edf4c35422b7d678e32430fd642a1deb131e3594
subsection
14
40
A natural section of the projection
Recall from Definition REF that \mathrm {M}^{\prime }=\mathrm {M}^{\prime }(\mathsf {H}) is a mixed complex whose underlying chain complex is HH(\mathrm {M}^{\prime })\!=\!(\mathrm {E}(\mathsf {H})_\mathrm {norm},\partial ^{\prime }), and write \pi ^{\prime } for the projection from the negative cyclic complex HN(\math...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 596, "openalex_id": "", "raw": "G. Ginot, Formules explicites pour le charactère de Chern en K-théorie algébrique, Ann. Inst. Fourier 54, (2004) 2327–2355.", "source_ref_id": "90b7f03f4d91ffb90669b344e6dfcb3da3c94021", ...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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0c67c6f96fb44f96e82e6022d829d25e706c69d2
subsection
15
40
A natural section of the projection
\quadThere is a sequence of \mathsf {H}-linear maps \Upsilon ^{\prime n}:\mathrm {E}(\mathsf {H})\rightarrow \mathrm {E}(\mathsf {H})[2n], starting with \Upsilon ^{\prime 0}=1, such that B^{\prime }(\Upsilon ^{\prime n}\,\partial ^{\prime }-\partial ^{\prime }\Upsilon ^{\prime n})=0.They induce maps on the normalized c...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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dad7dab2816488520ffd7b51ed091cd4289ab3ef
subsection
16
40
A natural section of the projection
By naturality of \kappa ^f in f, the above construction also goes through with \mathrm {E}(\mathsf {H}) replaced by M^{\prime }(\mathsf {H}), and the maps \Upsilon ^{\prime } on \mathrm {E}(\mathsf {H}) and HH(M^{\prime }) are compatible.We define maps \Upsilon ^{\prime }:HH(\mathrm {E}(\mathsf {H}))\rightarrow HN(\mat...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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a22584758a6f22bd9104c03869faa212173cc769
subsection
17
40
A natural section of the projection
Thus \Upsilon ^{\prime }(1)=(0,\dots ,0,1) in HN(M^{\prime }).Recall from Definition REF that M=k\otimes _{\mathsf {H}}M^{\prime }, and that \mathrm {B}(A)=k\otimes _A\mathrm {E}(A).There are morphisms of chain k-modules, \Upsilon \!:HH(\mathrm {B}(\mathsf {H}))\rightarrow HN(\mathrm {B}(\mathsf {H})) and \Upsilon \!:H...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
[ 12613, 41872, 53234, 172, 4759, 13331, 114654, 27750, 1369, 2389, 15464, 7, 6, 17727, 23, 79059, 132, 594, 8353, 85763, 155455, 9069, 919, 276, 92, 31, 70141, 420, 841, 4, 125458, 42, 39, 571, 8152, 284, 16, 647, 116959, 621, 178851, ...
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810d25535f456f6ec11d28e8154227cf1212d91f
subsection
18
40
The lift
Recall that C(\mathsf {H}) denotes the canonical cyclic complex of the algebra underlying \mathsf {H} (). We set \tau _0=\eta :k\rightarrow \mathsf {H}.Let \mathsf {H} be a cocommutative Hopf algebra. Then the k-linear map\tau :\mathrm {B}(\mathsf {H})\rightarrow C(\mathsf {H})\\ \tau (h_1\otimes \dots \otimes h_n)=S(h...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 105, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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6dd5c2b3576ef88dd05684f826334110659a91f6
subsection
19
40
Passage to completion
If A is a filtered algebra, the induced filtration (REF ) on the canonical cyclic module C(A) makes it a cyclic filtered module. Passing to completion we obtain a cyclic module C^{\rm top}(\hat{A}) with C^{\rm top}_n(\hat{A})=\hat{A}^{\hat{\otimes }n+1}. In the spirit of subsection REF , we write HH^{\rm top}(\hat{A}),...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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dafb5972567a11336432a3b6e16c9ae1258c4286
subsection
20
40
The case of universal enveloping algebras of Lie algebras
Let \mathfrak {g} be a Lie algebra over a commutative ring k. Then the enveloping algebra U\mathfrak {g} is a cocommutative Hopf algebra, so the constructions of the previous sections apply to U\mathfrak {g}. In particular a natural map c:\mathrm {B}(U\mathfrak {g})\rightarrow HN(U\mathfrak {g}) was constructed in (REF...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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36e66b68f56dc73a598acead7ee3a7dea3550e7a
subsection
21
40
Chevalley-Eilenberg complex
The Chevalley-Eilenberg resolution of k as a U\mathfrak {g}-module has the form (U\mathfrak {g}\otimes \wedge \mathfrak {g},d^{\prime }), and is given in . Tensoring it over U\mathfrak {g} with k, we obtain a complex (\wedge \mathfrak {g},d). Kassel showed in that the anti-symmetrization mape:\wedge ^n\mathfrak {g}\rig...
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0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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af134f86ba1dfccabde643dcb65c2f513cd5a98b
subsection
22
40
Chevalley-Eilenberg complex
Thus both 1\otimes e and e induce morphisms of mixed complexes U\mathfrak {g}\otimes \wedge \mathfrak {g}\rightarrow \mathrm {M}^{\prime }(U\mathfrak {g}) and \wedge \mathfrak {g}\rightarrow \mathrm {M}^{\prime }(U\mathfrak {g}).The diagrams{ U\mathfrak {g}\otimes \wedge \mathfrak {g}[d]_{1\otimes e}[r]^-{\psi ^{\prime...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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8eb5e4e91f849f320d0dd7305af9a510f48b5371
subsection
23
40
Chevalley-Eilenberg complex
By definition (see REF ),\tau =(S\otimes 1^{\otimes n})\circ (\nabla ^{(n)}\otimes 1^{\otimes n})\circ \sigma \circ \Delta ^{\otimes n}in C(U\mathfrak {g}). Since the x_i are primitive,\Delta ^{\otimes n}(x_1\otimes \dots \otimes x_n)=(x_1\otimes 1+ 1\otimes x_1)\otimes \dots \otimes (x_n\otimes 1+1\otimes x_n)Expandin...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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220fa0c1bba9ee7f3402238780dbbc2cd14c6da1
subsection
24
40
The Loday-Quillen map
We can now show that \tau \,\psi factors through the Connes' complex C^\lambda (U\mathfrak {g})=\operatorname{coker}(1-t:U^{\otimes \ast }\rightarrow HH(U\mathfrak {g})). We have a homomorphism \theta which lifts the Loday-Quillen map of to U\mathfrak {g}:\theta :\wedge ^{n+1}\mathfrak {g}\rightarrow C^\lambda _{n}(U\m...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 425, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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d9746e5bf21e9431db9ac39e30caaf964e7299a2
subsection
25
40
The Loday-Quillen map
The following result is implicit in the proof of for r=1, A=U\mathfrak {g}.\theta is a chain homomorphism \wedge \mathfrak {g}\rightarrow C^\lambda (U\mathfrak {g})[-1].To show that b\theta =-\theta d, we fix a monomial x_1\wedge \dots \wedge x_n and compute that b\theta (x_0\wedge \dots \wedge x_n)=\sum _{\sigma \in ...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 171, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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d855c62131bbb29c42311ef90c0eac9cffdc24e6
subsection
26
40
The Loday-Quillen map
Therefore b\theta (x_0\wedge \dots \wedge x_n)=-\theta d(x_0\wedge \dots \wedge x_n).Warning: the sign convention used for d in differs by -1 from the usual convention, used here and in and .It is well known and easy to see that, because Connes' operator B vanishes on the image of 1-t, it induces a chain map for ever...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 193, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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02afd77387840ad11386c9aae216160875b5bbeb
subsection
27
40
The Loday-Quillen map
We may interpret \theta (x_1\wedge \dots \wedge x_n) as the shuffle product x_1\star B(x_2)\star \dots \star B(x_n) (see ), and the nonzero coordinate of (REF ) as the shuffle product(1\otimes x_1)\star \dots \star (1\otimes x_n) =B(x_1)\star \dots \star B(x_n) \qquad \qquad \\ ~=~ B\bigl (x_1\star B(x_2)\star \dots \s...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 459, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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d4858b3ca8d93fb9304d10e8f6ba1b9812737f6e
subsection
28
40
Nilpotent Lie algebras and nilpotent groups
In this and the remaining sections we shall fix the ground ring k=\mathbb {Q}. Let \mathfrak {g} be a nilpotent Lie algebra; consider the completion \hat{U}\mathfrak {g} of its enveloping algebra with respect to the augmentation ideal, and setG=\exp {\mathfrak {g}}\subset \hat{U}\mathfrak {g}.This is a nilpotent group,...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 554, "openalex_id": "", "raw": "D. Quillen, Rational Homotopy Theory, Annals Math. 90 (1969), 205–295.", "source_ref_id": "ef1421e0ccde7a51d605d7a4ad7d13816a41f7f6", "start": 371 }, { "arxiv_id": "", ...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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176abc85de04762da39ce31ced83b566dd96a794
subsection
29
40
Nilpotent Lie algebras and nilpotent groups
Thus it suffices to show that the composite \mathrm {E}(\mathbb {Q}[G])\rightarrow \mathrm {E}^{\rm top}(\hat{\mathsf {H}}) is naturally homotopic to the map induced by the homomorphism \mathbb {Q}[G]\rightarrow \hat{\mathsf {H}}. By definition, these maps agree on \mathrm {E}_0(\mathbb {Q}[G]); thus their difference g...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1048, "openalex_id": "", "raw": "A. Suslin and M. Wodzicki, Excision in algebraic K-theory, Annals Math. 136 (1992) 51-122.", "source_ref_id": "61429a7c73e05702e5186f0f12b4b707ff9aadc3", "start": 552 } ] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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3414d639ecda8f1544b6f5ee2c97cece07048ef2
subsection
30
40
Nilpotent Lie algebras and nilpotent groups
Consider the resulting mapj:HN(\mathbb {Q}[G],\mathcal {I}_G)\rightarrow HN(\hat{U}\mathfrak {g},\hat{\mathcal {I}})\rightarrow HN(A,J).Putting together Theorem REF with Proposition , we get a naturally homotopy commutative diagram (with G=(1+J)^\times ):{ \mathrm {B}(\mathbb {Q}[G],\mathcal {I}_G)[r]^-{c}[d]_{sw}& HN(...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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c4617fbb76d201b2cd2d190a0a1ecc495f63ca6c
subsection
31
40
The relative Chern character of a nilpotent ideal
In this section we establish Theorem REF , promised in (REF ), that the two definitions (REF ) and (REF ) of the Chern character K_*(A,I)\rightarrow HN_*(A,I) agree for a nilpotent ideal I in a unital \mathbb {Q}-algebra A. The actual proof is quite short, and most of this section is devoted to the construction of the ...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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6631b98ba4486b38c70351ce86857545f2d937aa
subsection
32
40
The absolute Chern character
Let A be a unital \mathbb {Q}-algebra, and \mathrm {B}\mathrm {GL}(A) the classifying space of GL(A). Now the plus construction \mathrm {B}\mathrm {GL}(A)\rightarrow \mathrm {B}\mathrm {GL}(A)^+ is a homology isomorphism, and K_n(A)=\pi _n\mathrm {B}\mathrm {GL}(A)^+ for n\ge 1. In particular, the singular chain comple...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1036, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", ...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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bddd95ebafe68a238e792faeff985e00b7256350
subsection
33
40
The absolute Chern character
Composing this with the maps HN(A)\rightarrow HC(A)[2n] yields the map ch_{0,n}: K_0(A)\rightarrow HC_{2n}(A) of . From Example REF above, with A=k, we see that ch([k])=c(1), and ch_{0,n}([k])=(-1)^n(2n)!/n! in HC_{2n}(k)\cong k, in accordance with .
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 114, "openalex_id": "", "raw": "J.-L. Loday, Cyclic homology, volume 301 of Grundlehren der Mathematischen Wissenschaften, Springer-Verlag, Berlin, 1992.", "source_ref_id": "4e2dbed3573611a3de2e60d27f3010d74205db24", "...
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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ad938db4039e52ee90c791386656f8a71ff12918
subsection
34
40
Volodin models for the relative Chern character of nilpotent ideals
In order to define the relative version ch_* of the absolute Chern character, we need to recall a chunk of notation about Volodin models. For expositional simplicity, we shall assume that I is a nilpotent ideal in a unital \mathbb {Q}-algebra A.Let I a nilpotent ideal in a \mathbb {Q}-algebra A, and \sigma a partial or...
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0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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6f0c517a0ddd14e4db9d3ecf8bf68d37d1af6196
subsection
35
40
Volodin models for the relative Chern character of nilpotent ideals
On the other hand, by Example , we also have a mapC(\mathbb {Q}[G],\mathcal {I}_{G}) \ {j \over \longrightarrow }\ C(G), \quad \text{for~} G=\mathcal {T}_n^\sigma (A,I).From the definition of ch^-_A in (REF ) and the naturality of c, we obtain the promised description of ch^-, which we record.Set G=T_n^\sigma (A,I). Th...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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39d2b6521cf116ad07d335b9da6ef9a07d85b116
subsection
36
40
The relative Chern character for rational nilpotent ideals
When I is a nilpotent ideal in an algebra A, we define K(A,I) to be the homotopy fiber of B\mathrm {GL}(A)^+\rightarrow B\mathrm {GL}(A/I)^+; K(A,I) is a connected space whose homotopy groups are the relative K-groups K_n(A,I) for all n. We now cite Theorem 6.1 of for nilpotent I; the proof in is reproduced on page 36...
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0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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68bb2a614b1920cb080660e07855adaf36424df4
subsection
37
40
The rational homotopy theory character for nilpotent ideals
For a nilpotent ideal I, consider the chain subcomplex of the Chevalley-Eilenberg complex \wedge \mathfrak {gl}(A),x(A,I)=\sum _{n,\sigma } \wedge \mathfrak {t}_n^\sigma (A,I).Because sw is natural in G, the family of maps \mathrm {B}(\mathbb {Q}[T_n^\sigma (A,I)])\ {sw \over \longrightarrow }\ \wedge \mathfrak {t}_n^\...
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0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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882a4fa99fea6cfe09767e6ead092baeb5d4f48f
subsection
38
40
Main theorem
Let I be a nilpotent ideal in a \mathbb {Q}-algebra A. The relative Chern character ch of Definition REF induces the relative Chern character ch_* of (REF ) on homotopy groups, and the rational homotopy character ch^{\prime } of Definition REF induces the character ch^{\prime }_* of (REF ) on homotopy groups. Therefore...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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71043cff195759957fc15d3a74c2c584820a36fe
subsection
39
40
Naturality
In order to formulate a naturality result for the homotopy between ch and ch^{\prime }, it is necessary to give definitions for the maps ch and ch^{\prime } which are natural in A and I. Contemplation of Definitions REF and REF shows that we need to find a natural inverse for the backwards quasi-isomorphism of Theorem ...
{ "cite_spans": [] }
0807.1811
Relative Chern characters for nilpotent ideals
[ "Guillermo Cortiñas", "Charles Weibel" ]
[ "math.KT", "math.QA" ]
2,008
en
Mathematics
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974c2ea7c71e6aa34b9b36234ff4a5de10e1c0c6
abstract
0
9
Abstract
Let $\Omega$ be a two-dimensional heat conduction body. We consider the problem of determining the heat source $F(x,t)=\varphi(t)f(x,y)$ with $\varphi$ be given inexactly and $f$ be unknown. The problem is nonlinear and ill-posed. By a specific form of Fourier transforms, we shall show that the heat source is determine...
{ "cite_spans": [] }
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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e85f1edeacf81c12903356463e5487d25a724884
subsection
1
9
Body
Determine the source term of a two-dimensional heat equation DANG DUC TRONG ^1,  TRUONG TRUNG TUYEN ^2,PHAN THANH NAM ^1 and ALAIN PHAM NGOC DINH ^3^1 Mathematics Department, Natural Science HoChiMinh City University, Viet Nam^2 Mathematics Department, Indiana University, Rawles Hall , Bloomington, IN 47405^3 Mathemati...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1925, "openalex_id": "", "raw": "J.R.Cannon, S.Peùrez Esteva, Some stability estimates for a heat source in terms of over specified data in the 3-D heat equation, J. Math. Anal. Appl. 147(2)(1990) 363-371.", "source_ref_id":...
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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ce3c0c1e9aa2772f09de1d7c2f34a13c2696675d
subsection
2
9
Body
If (u_i,f_i) (i=1,2) satisfy the system (1) with g_0,g_1\in L^2(\Omega ) and \varphi \in L^1 (0,1)\backslash \lbrace 0\rbrace thenWe also have a regularization result. Using the Tikhonov regularization and truncated integration, we can construct a regularized solution for all \varphi \lnot \equiv 0.Theorem 2 (Regulariz...
{ "cite_spans": [] }
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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8674f1a5db40bec3254504ed6ac9dc49d6b2a739
subsection
3
9
Body
Let g_{\varepsilon }=(g_{0\varepsilon },g_{1\varepsilon })\in (L^2(\Omega ))^2 and \varphi _{\varepsilon }\in L^1 (0,1) be measured data satisfyingF̉rom \lbrace g_{0\varepsilon },g_{1\varepsilon },\varphi _{\varepsilon }\rbrace , we can construct a regularized solution f_{2\varepsilon }\in L^2(R^2) such thatM̉oreover, ...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1494, "openalex_id": "", "raw": "Dang Duc Trong and Truong Trung Tuyen, Error of Tikhonov's regularization for intergral convolution equations, preprint, available online at arXiv (2006).", "source_ref_id": "251b09b085b32771...
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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e9a27c152169290e33c833e1082153daee643df3
subsection
4
9
Body
Hence, for each n\in Z, the functionis also a nontrivial entire function.(i) For each n\in Z, since the zeros set of \phi _n is either finite or countable, D(\varphi )(\alpha ,n)=\phi _n(\alpha )\ne 0 for a.e \alpha \in R. Hence D(\varphi )(\alpha ,n)\ne 0 for all n\in Z and for a.e \alpha \in R.T̉o estimate the measur...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 422, "openalex_id": "", "raw": "B.Ya.Levin, Lectures on Entire Functions, Trans. Math. Monographs, Vol.150, AMS, Providence, Rhole Island (1996).", "source_ref_id": "28134eec222151933edb17df609832a5058c5658", "start": ...
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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c8e276cf393f57d09282176ecdc3dd5d66eb3455
subsection
5
9
Body
Thusfor \varepsilon >0 small enough (depended on \varphi , q and \beta ).(ii) Note thatTherefore, there exists a constant R_1>0 (depended on \varphi , \lambda ) satisfying for either |\alpha |\ge R_1 or |n|\ge R_1 thatConsequently, for \varepsilon >0 small enough (depended on \varphi , q and q_1) and for all (\alpha ,n...
{ "cite_spans": [] }
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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ea50504d8c60d84b64f288e20c613b716a90e1c7
subsection
6
9
Body
Moreover, if w\in H^1(\Omega ) thenFor each w\in L^2(\Omega ), applying Lemma 4 we obtainIt implies that \mathop {\lim }\limits _{r \rightarrow + \infty } \mu (w,r) = 0.N̉ow, we consider w\in H^1(\Omega ). Sincewe getConsequently,Similarly, we haveTherefore,HenceNoting thatwe getandThusIn summary, we getT̉he proof is c...
{ "cite_spans": [] }
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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92c298d71766a1bbf9bb80690f95c92bc59670a2
subsection
7
9
Body
We haveWe getand similarly,Thus,We next considerIf \left| {D(\varphi _{ex} )} \right| \ge \varepsilon ^q thenIf \left| {D(\varphi _{ex} )} \right|<\varepsilon ^q thenwhere B(\varphi _{ex} ,R_\varepsilon ,\varepsilon ^q) is as in Definition 1.Ỉn summary, for all (\alpha ,n)\in R \times Z , we haveTo estimate \sum \limit...
{ "cite_spans": [] }
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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d28c3fb73edc92827c1fc113a784ec7aabfe6e8d
subsection
8
9
Body
A numerical experimentWe consider the exact dataThen the corresponding exact solution of the system (1) isFor all m=2,4,6,8,..., we consider the disturbed dataThen the corresponding disturbed solution of the system (1) isWe getIt means that, when m is large, a small error of data causes a large error of solution. Hence...
{ "cite_spans": [] }
0807.1812
Determine the source term of a two-dimensional heat equation
[ "Dang Duc Trong", "Truong Trung Tuyen", "Phan Thanh Nam", "Alain Pham Ngoc Dinh" ]
[ "math.AP" ]
2,008
en
Mathematics
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c36678972b17b8773d98af69645e8986370c9a83
abstract
0
29
Abstract
The aim of this paper is to provide a logic-based conceptual analysis of the twin paradox (TwP) theorem within a first-order logic framework. A geometrical characterization of TwP and its variants is given. It is shown that TwP is not logically equivalent to the assumption of the slowing down of moving clocks, and the ...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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1b90d652b58a03daa6028fab44297aa49c8caa1b
subsection
1
29
Introduction
The twin paradox (TwP) theorem is one of the most famous predictions of special relativity. According to TwP, if a twin makes a journey into space, he will return to find that he has aged less than his twin brother who stayed at home. However surprising TwP is, it is not a contradiction. It is only a fact that shows th...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1184, "openalex_id": "", "raw": "H. Andréka, J. X. Madarász, and I. Németi. Logic of space-time and relativity theory. In M. Aiello, I. Pratt-Hartmann, and J. van Benthem, editors, Handbook of spatial logics, pages 607–711. Spring...
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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ae91875eb6317676bc3adac8bc35fd65a665b54b
subsection
2
29
Introduction
The linearity of transformations between inertial observers (inertial reference frames) can also be proven from some plausible assumptions, therefore it need not be assumed as an axiom, see , .The usual approaches to special theory of relativity base the theory on two postulates, namely, Einstein's principle of relativ...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 193, "openalex_id": "", "raw": "H. Andréka, J. X. Madarász, and I. Németi. On the logical structure of relativity theories. With contributions from: A. Andai, G. Sági, I. Sain and Cs. Tőke. research report, Alfréd Rényi Institute ...
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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86ce4e678f4d9f41e2bc22eb6e98b3c33bd9be38
subsection
3
29
Introduction
Hilbert's 6th problem . In our perspective axiomatization is only a first step to logical and conceptual analysis where the real fun begins.For good reasons, the foundation of mathematics was performed strictly within FOL. A reason for this fact is that staying within FOL helps to avoid tacit assumptions. Another reaso...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 544, "openalex_id": "", "raw": "H. Andréka, J. X. Madarász, and I. Németi. On the logical structure of relativity theories. With contributions from: A. Andai, G. Sági, I. Sain and Cs. Tőke. research report, Alfréd Rényi Institute ...
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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9a7edfb157c620e1f3fad811a0d31d992588864c
subsection
4
29
A FOL axiom system of kinematics
Here we explain our basic concepts. We deal with kinematics, i.e., with the motion of bodies (anything which can move, e.g., test-particles, reference frames, electromagnetic waves or centers of mass). We represent motion as the changing of spatial location in time. Thus we use reference frames for coordinatizing event...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 706, "openalex_id": "", "raw": "J. Ax. The elementary foundations of spacetime. Found. Phys., 8(7-8):507–546, 1978.", "source_ref_id": "edd920ef4998f3b7bda740323444ba7a8a8b4ad0", "start": 649 }, { "arxiv_...
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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4e6cd9d7e1a776114c6e30841fcc660b5a045b9f
subsection
5
29
A FOL axiom system of kinematics
\mathsf {IOb}(m), \mathsf {W}(m,b,x_1,\ldots , x_d), m=b, x_1=x_2 and x_1<x_2 are the so-called atomic formulas of our FOL language, where m,b,x_1,\dots ,x_d can be arbitrary terms of the required sorts. The formulas of our FOL language are built up from these atomic formulas by using the logical connectives not (\lnot...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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9b38b025b8eccbd7b5ebef52e5faf463f71d0db5
subsection
6
29
A FOL axiom system of kinematics
If p\in \mathsf {Q}^n, we assume that p=\langle p_1,\ldots ,p_n\rangle , i.e., p_i\in \mathsf {Q} denotes the i-th component of the n-tuple p. Specially, we write \mathsf {W}(m,b,p) in place of \mathsf {W}(m,b,p_1,\dots ,p_d), and we write \forall p in place of \forall p_1\dots \forall p_d, etc. To abbreviate formulas,...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1276, "openalex_id": "", "raw": "C. C. Chang and H. J. Keisler. Model theory. North-Holland Publishing Co., Amsterdam, 1990.", "source_ref_id": "2d54245bc986ec093857677736326459a3268f9a", "start": 1214 } ] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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442821af7803dde34fd4057bbe9c705d76321df3
subsection
7
29
A FOL axiom system of kinematics
The set of positive elements of \mathsf {Q} (i.e., the set \lbrace x\in \mathsf {Q}:0<x\rbrace ) is denoted by \colorbox {defbgcolor}{\mathsf {Q}^+}. [Figure: Illustration of the basic definitions]We need some definitions and notations to formulate our other axioms. The set \mathsf {Q}^d is called the coordinate system...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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2d99d2e093722875777e8af430778f11fcfd2ac9
subsection
8
29
A FOL axiom system of kinematics
Let Ev_m denote the set of nonempty events coordinatized by observer m, i.e.,\colorbox {defbgcolor}{Ev_m}\,\mbox{$:=$}\,\left\lbrace \,\mathsf {ev}_m(p) \::\: \mathsf {ev}_m(p)\ne \emptyset \,\right\rbrace ,and Ev denote the set of all observed events, i.e.,\colorbox {defbgcolor}{Ev}\,\mbox{$:=$}\,\left\lbrace \,e\in E...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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5cdb036db10ee87a10e0cebbace5339647d826b3
subsection
9
29
A FOL axiom system of kinematics
Let us note that whenever we write \mathsf {time}_m, we assume that the events in its argument have unique coordinates by Convention REF .The coordinate-domain of observer m, in symbols Cd_m, is the set of coordinate points where m observes something, i.e.,\colorbox {defbgcolor}{Cd_m}\,\mbox{$:=$}\,\lbrace \, p\in \mat...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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6a750f76a2144ab9e27d6888c7a33ab76b7ba6fa
subsection
10
29
A FOL axiom system of kinematics
The time-unit vector of k according to m is defined as\colorbox {defbgcolor}{1^k_m}\,\mbox{$:=$}\,w^k_m(1_t)-w^k_m(o).The world-line of body b according to observer m is defined as the set of coordinate points where b was observed by m, i.e.,\colorbox {defbgcolor}{\mathsf {wl}_m(b)}\,\mbox{$:=$}\,\lbrace \, p\in \maths...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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f9754db132f0d71d73ffa414fd06ab943a6189e5
subsection
11
29
Geometrical Characterization of TwP
Since the axiom systems we use here deal only with inertial motions of observers, we formulate the inertial version of TwP, which is also called clock paradox in the literature.This inertial version is the one that was formulated by Einstein in his famous 1905 paper, see . Logical investigation of the accelerated versi...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
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2309238b2bd8062e4d5f03bdccce2ebf2a3a7465
subsection
12
29
Geometrical Characterization of TwP
That does not mean abandoning our FOL language. It is just simplifying the formalization of our axioms. Instead of events we could speak about observers and spacetime locations. For example, instead of \forall e\in Ev_m\phi we could write \forall p\in Cd_m\phi [e\!\leadsto \! \mathsf {ev}_m(p)], where none of p_1\ldots...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
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Physics
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c07df70e085873fb9327dcf795772e875252cf3f
subsection
13
29
Geometrical Characterization of TwP
Then&\mathsf {time}(\widehat{ac}<b)(e_a,e,e_c) &\quad &\Longleftrightarrow \ &\quad &\mathsf {Conv}({}^\ddag 1_m^a,{}^\ddag 1_m^b,{}^\ddag 1_m^c),\\ &\mathsf {time}(\widehat{ac}=b)(e_a,e,e_c) & &\Longleftrightarrow \ & &\mathsf {Bw}({}^\ddag 1_m^a,{}^\ddag 1_m^b,{}^\ddag 1_m^c),\\ &\mathsf {time}(\widehat{ac}>b)(e_a,e,...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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63805e9a83ae849d9335ad87ca815f692b6e59d2
subsection
14
29
Geometrical Characterization of TwP
From which, by axcolor\mathsf {AxLinTime}, it follows that\Big |\mathsf {time}_a(e_a,e)\Big |+\Big |\mathsf {time}_c(e,e_c)\Big | = \frac{|p-q|}{|a^\ddag |}+\frac{|q-r|}{|c^\ddag |}\\ =\frac{|p-s|+|s-r|}{|b^\ddag |}=\frac{|r-p|}{|b^\ddag |}= \Big |\mathsf {time}_c(e_a,e_c)\Big |.Hence \mathsf {time}(\widehat{ac}=b)(e_a...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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445c7329707c64a40cf4a5e65b843cf6b7d30f08
subsection
15
29
Geometrical Characterization of TwP
By the respective definitions, it is easy to see that any nontrivial convex (flat, concave) set intersects a halfline at most once.Let us define the Minkowski sphere here as \colorbox {defbgcolor}{MS^\ddag _m}\,\mbox{$:=$}\,\big \lbrace \, {}^\ddag 1^k_m \::\: k\in \mathsf {IOb}\,\big \rbrace .Remark 3 Convexity as use...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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c85ed1a9dec90c68df1e65644a2f382fd39349e8
subsection
16
29
Geometrical Characterization of TwP
Now we can reverse the implications of Corollary REF .Theorem 1 Assume axcolor\mathsf {Kinem_0} and axcolor\mathsf {AxShift}. Then&{axcolor}{\mathsf {TwP}} &&\Longleftrightarrow \ && \forall m\in \mathsf {IOb}MS^\ddag _m \text{ is convex,}\\ &{axcolor}{\mathsf {noTwP}} & &\Longleftrightarrow \ & &\forall m\in \mathsf ...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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9a364e342c88a793cb171f0a45b0d53f1252b44f
subsection
17
29
Consequences for Newtonian kinematics
Let us investigate the logical connection between No-TwP and the Newtonian assumption on the absoluteness of time.axcolor\mathsf {AbsTime} Observers measure the same time elapsing between events: \forall m,k\in \mathsf {IOb}\forall e_1,e_2\in Ev\quad \mathsf {time}_m(e_1,e_2)=\mathsf {time}_k(e_1,e_2).To strengthen ou...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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f8bc7a269d766c36e960ebe7fbdc90d9ad3b945e
subsection
18
29
Consequences for Newtonian kinematics
A more experimental version of axiom axcolor\mathsf {AxThExp^+} is the following:axcolor\mathsf {AxThExp^*} Observers can move in any direction at a speed which is arbitrarily close to any finite speed: \forall m\in \mathsf {IOb}\forall p,q\in \mathsf {Q}^d\forall \varepsilon \in \mathsf {Q}^+ \quad p_\tau \ne q_\tau...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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8a6cd26a433886dc9d48ce3237999bea1bd43b2f
subsection
19
29
Consequences for Newtonian kinematics
If the hyperplane containing MS^\ddag _m were not horizontal, there would be nonhorizontal lines parallel to it. Therefore MS^\ddag _m has to be a subset of a horizontal hyperplane. If MS^\ddag _m were a porper subset of this hyperplane, there would be nonhorizontal lines not intersecting it. So MS^\ddag _m has to be a...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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410113b1c68138e34ec321e925e5ebf0c2c56a66
subsection
20
29
Consequences for Newtonian kinematics
Hence axcolor\mathsf {AbsTime} is not true in this model, as we claimed.
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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717646c094f9f443e4060645c0ad5a963ebe73ac
subsection
21
29
Consequences for special relativity theory
Now we are going to investigate the consequences of Theorem REF for special relativity. To do so, let us extend our language by a new unary relation \mathsf {Ph} on \mathsf {B} for photons (light signals) and formulate an axiom on the constancy of the speed of light. For convenience, this speed is chosen to be 1.axcolo...
{ "cite_spans": [] }
10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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bdbab3c4fd2a661368a2a4bceba10fa0b475eb35
subsection
22
29
Consequences for special relativity theory
Every bijection from F^d to F^d that transforms lines of slope 1 to lines of slope 1 is a Poincaré transformation composed by a dilation and a field-automorphism-induced map.For the proof of Theorem REF , see , . From this theorem we derive that the worldview transformations between observers are Poincaré ones in the m...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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f19392b8902fa8218420456e5da1083e177900d5
subsection
23
29
Consequences for special relativity theory
Hence w^k_m is a Poincaré transformation.Let us now formulate another famous prediction of relativity.axcolor\mathsf {SlowTime} Relatively moving observers' clocks slow down: \forall m,k\in \mathsf {IOb}\quad \mathsf {wl}_m(k)\ne \mathsf {wl}_m(m) \rightarrow \big |(1^k_m)_\tau \big |>1.To investigate the logical conn...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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f93e1123d95f321fb2cb888555e999e4a7802dea
subsection
24
29
Consequences for special relativity theory
Hence \mathsf {time}_m(e) is between \mathsf {time}_m(e_a) and \mathsf {time}_m(e_c) iff \mathsf {time}_b(e) is between \mathsf {time}_b(e_a) and \mathsf {time}_b(e_c). This completes the proof since the other parts of the definition of relation \mathsf {meetTwP} do not depend on observers m and b.We cannot consistentl...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
en
Physics
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178ffca9d6cacfa8fecdfd8ea0cfd8d1c8197e36
subsection
25
29
Consequences for special relativity theory
Let \mathsf {IOb}\,\mbox{$:=$}\,\lbrace \langle p,q\rangle \in \mathsf {B}\,:\,|p_\sigma -q_\sigma |<|p_\tau -q_\tau |\rbrace . It is easy to see that there is a nontrivial convex subset M of \mathsf {Q}^d such that 1_t\in M and |p_\tau |<1 for some p\in M. Let MS^\ddag _{\langle 1,0\rangle } be such a convex subset of...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
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1f1b31de23f57583892da4ce0b0ac8f58394bf9b
subsection
26
29
Consequences for special relativity theory
Then{axcolor}{\mathsf {SpecRel^-_\mathit {d}}}+{axcolor}{\mathsf {AxSymDist}}&\models {axcolor}{\mathsf {TwP}}, \text{ but}\\ {axcolor}{\mathsf {SpecRel^-_\mathit {d}}}+ {axcolor}{\mathsf {AxShift}}+{axcolor}{\mathsf {AxLinTime}} +{axcolor}{\mathsf {AxThExp}}+{axcolor}{\mathsf {TwP}}&\lnot \models {axcolor}{\mathsf {A...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
2,008
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46ad8c5a3d20aa676119d56eee299be1908de87e
subsection
27
29
Consequences for special relativity theory
This theorem is interesting because it shows that assuming only that all moving clocks slow down to some degree implies the exact ratio of the slowing down of moving clocks (since if \mathit {d}\ge 3, {axcolor}{\mathsf {SpecRel^-_\mathit {d}}}+{axcolor}{\mathsf {AxSymDist}} implies that the worldview transformations ar...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
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3978aa70082c0c6dfb9900bbee737a12647a4bbc
subsection
28
29
Concluding remarks
We have seen that (the inertial version of) TwP can be characterized geometrically within a general axiom system of kinematics. We have also seen some surprising consequences of this characterization; in particular, that TwP is logically weaker than axiom axcolor\mathsf {AxSymDist} of special relativity as well as the ...
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10.1007/s11225-010-9253-7
0807.1813
A Geometrical Characterization of the Twin Paradox and its Variants
[ "Gergely Szekely" ]
[ "math-ph", "gr-qc", "math.LO", "math.MP" ]
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0bd8fdb6c5af3f42529205e0e3a4dec67c7c09dd
abstract
0
9
Abstract
A growing or shrinking disc will adopt a conical shape, its intrinsic geometry characterized by a surplus angle $se$ at the apex. If growth is slow, the cone will find its equilibrium. Whereas this is trivial if $se <= 0$, the disc can fold into one of a discrete infinite number of states if $se$ is positive. We constr...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
2,008
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6218d16f4a09dfdf29bad04b13b88742a0a84c32
subsection
1
9
Body
Conical defects in growing sheetsMartin Michael Müller Martine Ben Amar Laboratoire de Physique Statistique de l'Ecole Normale Supérieure (UMR 8550), associé aux Universités Paris 6 et Paris 7 et au CNRS; 24, rue Lhomond, 75005 Paris, FranceJemal Guven Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de M...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
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96ca155d6c669203ac94c200290edb6b47c9b2ac
subsection
2
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Body
Whereas this state is an unremarkable circular cone in the case of a deficit, when the deficit is turned to surplus, the folded shape–an excess-cone (e-cone for short)–exhibits a surprisingly subtle behavior. In this letter, we will describe the equilibrium states associated with these “point defects” in the full nonli...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
2,008
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subsection
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The constraint of unstretchability is implemented by adding a term to the energy functional which fixes the metric via a set of local Lagrange multipliers T^{ab} . These can be identified with a conserved tangential stress.The shape equation and its solution. There is a remarkably simple way to determine the shape of t...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
2,008
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a75f8bc0d114b8ae0a0ec967ce861db3f652789a
subsection
4
9
Body
For small \varphi _{\text{e}}, we find k=a_{1}\varphi _{\text{e}}+{\mathcal {O}}(\varphi _{\text{e}}^{2}), where a_{1} = -\frac{1}{2\pi }(1-\frac{1}{n^{2}}). [Figure: Paper model (a) and calculated surface shapes for \varphi _{\text{e}}=2\pi with n=2 (b),n=3 (c), and n=4 (d).]Surface shapes. The e-cone has to have two ...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
2,008
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b25aa86ecf9c9fa60fe33d630a7bfc85b2346d6c
subsection
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REF the values of \varphi _{\text{e}}^{\text{kiss}} of various n-folds are given. [Table: Kissing points for different n-folds.]Interestingly, \varphi _{\text{e}}^{\text{kiss}} converges to \varphi _{\text{e}, \text{max}}^{\text{kiss}}\approx 35.23 from below if n is sent to infinity. This implies that one cannot find ...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
2,008
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4342a137e1e682a2dbfc12312eade2bc7b4051d7
subsection
6
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Body
Investigated more carefully, however, a set of adjacent intersection points is found which converge to \varphi _{\text{e}}\approx 7.47 for n\rightarrow \infty . Above this region each curve reaches a maximum which diverges quadratically with n. If n>5 and \varphi _{\text{e}} sufficiently large, C_{\Vert } is greater th...
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10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
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a3b05b095865334b1a143a0dbce5b75feb95d8e7
subsection
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Body
However, with increased crowding one begins to force up the average curvature: above \varphi _{\text{e}}=8.27 the 3-fold possesses lower energy than the touching symmetrical 2-fold and the e-cone may flip from n=2 to n=3. Equivalent behavior is expected if \varphi _{\text{e}} is increased. To analyze the stability of o...
{ "cite_spans": [] }
10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
2,008
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Physics
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173c9079ec09d81155b705442f4a102141b4f887
subsection
8
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These truncated cones can also be glued together to model surfaces which are not flat: a surface of constant negative Gaussian curvature can be approximated by a telescope formed by such annuli.Partial support from CONACyT grant 51111 as well as DGAPA PAPIIT grant IN119206-3 is acknowledged. The authors would like to t...
{ "cite_spans": [] }
10.1103/PhysRevLett.101.156104
0807.1814
Conical defects in growing sheets
[ "Martin Michael Mueller", "Martine Ben Amar", "Jemal Guven" ]
[ "cond-mat.other", "cond-mat.mtrl-sci", "cond-mat.soft" ]
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abstract
0
9
Abstract
Recently, Matzkin claimed the construction of a hidden variable (HV) model which is both local and equivalent with the quantum-mechanical predictions. In this paper we will briefly present this HV model and argue, by identifying an extra non-local "hidden" HV, why this model is not local
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
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e0245932ce723adbf2bbf3283fcfc41948d372b9
subsection
1
9
Introduction
With the derivation of his well-known inequalities, Bell proved that any local model based on hidden variables (HV) can not reproduce the empirical predictions of quantum-mechanics. Recently however, Matzkin claimed that he has constructed a HV model which is both local and equivalent with the quantum-mechanical predic...
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0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
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subsection
2
9
EPRB
In the EPRB-experiment, studied by both Bell and Matzkin, a pair of spin-\frac{1}{2} particles are formed in the singlet spin state \mathinner {|{\Psi _0}\rangle } :\mathinner {|{\Psi _0}\rangle } = \frac{1}{\sqrt{2}}( \mathinner {|{{z}\uparrow }\rangle } \otimes \mathinner {|{{z}\downarrow }\rangle } - \mathinner {|{{...
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 360, 70, 26201, 45176, 9, 230648, 22282, 15044, 33500, 136, 7656, 169, 875, 80836, 25927, 132076, 418, 304, 2878, 66695, 621, 100, 4806, 11001, 18, 11341, 4450, 13857, 172, 2389, 5445, 864, 31, 70141, 118201, 12647, 927, 25813, 4092, 1982...
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55500d2e9e82875961bffb87b4463e69da96686c
subsection
3
9
Matzkins HV model
Matzkins HV model makes use of the following elements:HV. A single particle is specified by a hidden variable \vec{\lambda }: a normalized vector in \mathbb {R}^3. For the two particles specified by (\vec{\lambda }_1, \vec{\lambda }_2) in the singlet spin state, anti-correlation is described by the relation: \vec{\lam...
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 7656, 23445, 1779, 101422, 3299, 30482, 4527, 111, 25632, 80854, 11001, 915, 26147, 58735, 204105, 77336, 35259, 6492, 85, 3638, 29367, 173, 18770, 5125, 1052, 363, 6626, 2878, 66695, 115187, 10461, 18, 25927, 11341, 2874, 32399, 57860, 15155...
[ 0.1336669921875, 0.189453125, 0.0980224609375, 0.2861328125, 0.2491455078125, 0.05908203125, 0.1483154296875, 0.0074462890625, 0.05010986328125, 0.1544189453125, 0.1767578125, 0.043792724609375, 0.18310546875, 0.191650390625, 0.197509765625, 0.1961669921875, 0.174560546875, 0.14794...
51107cf4355bc29ccd4d395000f659d18c198d0e
subsection
4
9
Matzkins HV model
For a system consisting of a single particle in a quantum state with a positive spin along the \vec{z}-axis (having an initial HV distribution R_{\pm \frac{1}{2}\vec{z}}) the probabilities of \mathcal {M}(R=R_{+\frac{1}{2}\vec{z}},\vec{u},\vec{\lambda }) = \pm \frac{1}{2} by measuring the spin component in direction \v...
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 1326, 5426, 58055, 11001, 915, 26147, 110436, 11341, 678, 24491, 25927, 33233, 35259, 169, 33102, 528, 61475, 101422, 113068, 627, 26822, 132076, 304, 37242, 31075, 125458, 6827, 594, 1328, 34, 143, 6492, 85, 163, 162, 82761, 48225, 34475, ...
[ 0.0084228515625, 0.177978515625, 0.054718017578125, 0.1251220703125, 0.051422119140625, 0.183837890625, 0.1441650390625, 0.11181640625, 0.013916015625, 0.1644287109375, 0.2171630859375, 0.06695556640625, 0.175537109375, 0.1048583984375, 0.1126708984375, 0.002532958984375, 0.090454101...
69fe03e1f37b87732d38fa4bc2c1a4bb0325e6e4
subsection
5
9
A HV model for two particles
With these elements a HV-model for the EPRB experiment is constructed. The system consists of two particles, described with the HV (\vec{\lambda }_1, \vec{\lambda }_2) respecting correlation (REF ). The initial distribution of HV for each particle in the singlet state is (as given by Matzkin) a uniform distribution R_{...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1942, "openalex_id": "", "raw": "J.S. Bell, Physics 1, 195 (1964).", "source_ref_id": "697b27ecb700bca8a162abd83e88da460af8e568", "start": 1809 } ] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 17106, 6097, 80854, 101422, 9, 51734, 100, 26201, 45176, 28007, 64549, 297, 5426, 58055, 111, 6626, 2878, 66695, 4, 151552, 6, 15, 35259, 24854, 143, 6492, 85, 51912, 115187, 41872, 454, 10461, 15072, 214, 16106, 57860, 11766, 919, 61475, ...
[ 0.040802001953125, 0.0145721435546875, 0.1490478515625, 0.31396484375, 0.017730712890625, 0.265625, 0.0154266357421875, 0.1142578125, 0.249755859375, 0.225830078125, 0.1107177734375, 0.010040283203125, 0.157958984375, 0.118408203125, 0.0305938720703125, 0.1204833984375, 0.15283203125...
d3f23432f799bb16ba9f167472fcd2566396e4cc
subsection
6
9
A HV model for two particles
Matzkin states that if we measure the spin component of particle 1 along axis \vec{a} (S_{\vec{a}}) and obtain, for example, result a = +\frac{1}{2}, we know (using (REF )) that \vec{\lambda }_1 \cdot \vec{a} \ge 0. With the anti-correlation (REF ) in mind, we therefore also know that \vec{\lambda }_2 \cdot \vec{a} \le...
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 7656, 169, 875, 117249, 2174, 72350, 25927, 82761, 915, 26147, 106, 33233, 33102, 6, 35259, 11, 8152, 294, 24854, 41872, 47391, 16, 113054, 4, 100, 27781, 16750, 10, 2203, 997, 132076, 418, 304, 3714, 223, 214, 11766, 919, 143, 6492, 85...
[ 0.1671142578125, 0.169189453125, 0.235107421875, 0.0902099609375, 0.04248046875, 0.226806640625, 0.236083984375, 0.220947265625, 0.045257568359375, 0.178955078125, 0.09906005859375, 0.0745849609375, 0.1065673828125, 0.002899169921875, 0.2318115234375, 0.07855224609375, 0.003112792968...
8840cf44c9be13b7d3be804f711b32bfe8e9fc01
subsection
7
9
A HV model for two particles
Both of these properties are in conflict with the definition of “locality” as given by Bell.Matzkin does not give us any local mechanism (based on information locally available) to explain the perturbation of the HV distribution of particle 2 after measuring particle 1. So, we have to conclude that the initial HV distr...
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 149766, 183871, 23, 79612, 80934, 98908, 2481, 34475, 33500, 79520, 169, 875, 959, 8337, 1821, 4000, 191619, 77007, 4677, 19882, 73342, 170950, 1363, 101422, 113068, 915, 26147, 116, 7103, 163, 162, 53089, 615, 103876, 61475, 627, 872, 192, ...
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c945eed7d24b6b72d1864a27feb76e3713664a83
subsection
8
9
Conclusion
We recognize that measurement outcomes in the HV model of Matzkin not only depend on the HV \vec{\lambda } and the the measurement direction \vec{u}, but also on a initial HV distribution R. In the HV model for the two particles in the EPRB experiment, the initial HV distribution of particle 2 is modified, based on bot...
{ "cite_spans": [] }
0807.1815
A local hidden-variable model violating Bell's inequalities: a reply to Matzkin
[ "R. N. Nijhoff" ]
[ "quant-ph" ]
2,008
en
Physics
[ 125296, 72350, 674, 184345, 7, 101422, 3299, 7656, 169, 875, 56566, 35259, 6492, 85, 48225, 34, 61475, 113068, 627, 6626, 2878, 66695, 26201, 45176, 28007, 915, 26147, 116, 83, 73197, 35509, 615, 149766, 183871, 79612, 678, 55738, 4000, 154...
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885e1dba3d533f656fca05fe2c0aff55223669af
abstract
0
8
Abstract
The presence of exponential bulges and anti-truncated disks has been noticed in many lenticular galaxies. In fact, it could be expected because the very formation of S0 galaxies includes various processes of secular evolution. We discuss how to distinguish between a pseudobulge and an anti-truncated disk, and also what...
{ "cite_spans": [] }
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 169424, 78643, 80973, 11876, 4188, 136, 2874, 9774, 16336, 3674, 28338, 1556, 156672, 5941, 121469, 25667, 22703, 5134, 15824, 5809, 84751, 70, 4552, 27643, 159, 2389, 90, 96853, 67842, 9433, 40, 137089, 45252, 3642, 157167, 1495, 17721, 7418...
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7dea0486fe02e9fd3cb575f7f9c7ec6434c7abce
subsection
1
8
Introduction
Bulges have been traditionally thought to have de Vaucouleurs' brightness profiles just as elliptical galaxies (e.g. ). However John Kormendy (, , ) has proved that there exists a type of bulges named `pseudobulges' which resemble disks from the dynamical point of view: they are rather cold and demonstrate fast rotatio...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 119, "openalex_id": "", "raw": "Freeman, K.C. 1970, ApJ 160, 811", "source_ref_id": "4d811bf2d7f6e55354139f2c11c49f3d6c38140d", "start": 0 }, { "arxiv_id": "", "doi": "", "end": 322, "op...
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 166599, 90, 765, 2809, 89160, 538, 17569, 8, 142672, 587, 202, 17706, 124498, 7432, 60641, 7, 1660, 237, 21392, 70760, 22703, 5134, 15, 13, 5, 6, 33306, 4939, 3970, 25965, 53, 4, 1388, 77443, 32316, 10644, 111, 11876, 4188, 4806, 45616,...
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3e99245c08f222ded1bf6a036517c06b638441c7
subsection
2
8
Introduction
But for face-on galaxies we can use kinematical data and estimate their thickness by measuring vertical stellar velocity dispersions.We have now started a program of studying systematically multi-tiers (anti-truncated) exponential structures in early-type, presumably lenticular, galaxies. The study will include photome...
{ "cite_spans": [] }
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 4966, 100, 2577, 191, 22703, 5134, 90, 642, 831, 4527, 200, 69131, 70760, 2053, 136, 25902, 67, 6117, 2594, 7432, 163, 162, 79259, 29486, 320, 191060, 225202, 12137, 5036, 26859, 1528, 35187, 214, 242161, 6024, 118, 1314, 5772, 9774, 1633...
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8525fc0f8c78bae650f34fd3d5c219c2a5e15b3a
subsection
3
8
Observations
The photometric observations the results of which we discuss here have been made with the focal reducer SCORPIO of the Russian 6m telescope () in the direct-image mode. The CCD detector EEV 42-40 with the size of 2048 \times 2048 has been used in binned mode of 2\times 2. The field of view was about 6 arcminutes, the s...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 168, "openalex_id": "", "raw": "Afanasiev, V.L. & Moiseev, A.V. 2005, Astronomy Letters 31, 194", "source_ref_id": "193d12ca2cd7588c04e13ccf7f6167213b45f202", "start": 0 } ] }
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 581, 16186, 186518, 150556, 7, 50339, 642, 45252, 3688, 765, 7228, 678, 89716, 34390, 42, 124853, 15185, 670, 102374, 305, 39, 5501, 70820, 8951, 37926, 13736, 16069, 96391, 748, 241, 40972, 4828, 41734, 13267, 387, 9285, 70141, 1556, 11814...
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67dea77b85de9debafd11ce67ef00fc8d249e513
subsection
4
8
Photometric structure of the central group S0 galaxies
Two central group galaxies under consideration are typical giant lenticular galaxies, with the blue absolute magnitudes of about -21.6 - -21.7 (HYPERLEDA). Both are very red, (B-V)_e=1.07, and are seen face-on, b/a>0.9.We have calculated azimuthally averaged surface brightness profiles for NGC 524 in two filters, B and...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 770, "openalex_id": "", "raw": "Baggett, W.E., Baggett, S.M., Anderson, K.S.J. 1998, AJ 116, 1626", "source_ref_id": "34ccb8fa67c31b68ed79bb597f33dc13d0bdc3e1", "start": 566 }, { "arxiv_id": "", "do...
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 32964, 9879, 21115, 22703, 5134, 90, 1379, 177229, 621, 222201, 6051, 18, 121469, 25667, 4, 678, 70, 57571, 89931, 101668, 111, 1672, 122297, 122336, 20, 133760, 92559, 30425, 38409, 284, 149766, 4552, 4842, 15, 571, 9, 856, 16, 454, 13, ...
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81f6605677d1b00654f3549024d2e64e90904e37
subsection
5
8
Photometric structure of the central group S0 galaxies
REF ). The profiles of the colour and of the stellar velocity dispersion are qualitatively similar! Certainly, we see a transition from the (exponential) bulge to the inner disk at R\approx 10^{\prime \prime }. Preliminary estimates of the scaleheight of the inner disk in NGC 524, by treating the measured line-of-sight...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 742, "openalex_id": "", "raw": "Sil'chenko, O.K., Koposov, S.E., Vlasyuk, V.V., Spiridonova, O.I. 2003, Astronomy Reports 47, 88", "source_ref_id": "4adc7f05ef89fc28c43665be92b411ee31fd2c96", "start": 502 } ] }
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 9069, 919, 194, 60641, 134855, 136, 29486, 320, 191060, 939, 225202, 191, 621, 150234, 21286, 21373, 38, 25500, 538, 4, 1957, 149307, 1295, 70, 157034, 19, 80973, 16, 11876, 429, 47, 75414, 28338, 99, 627, 2631, 64101, 209, 114654, 6, 1...
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a1adf10a9e8ed531d09c00b9ab71855becaacf56
subsection
6
8
What can be the mechanisms to form anti-truncated disks in lenticular galaxies?
It seems clear that anti-truncated disks are to be a result of matter re-distribution along the radius of a disk galaxy, and the very event of re-distribution must be rather fast and discrete. Several candidate mechanisms can be proposed. Younger et al. () simulates a minor merger, and they obtain an anti-truncated ste...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 455, "openalex_id": "", "raw": "Younger, J.D., Cox, T.J., Seth, A.C., Hernquist, L. 2007, ApJ 670, 269", "source_ref_id": "fb719ac92fab00eedbaf71c20907a4056348e1a8", "start": 239 } ] }
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 37202, 34735, 2874, 9774, 16336, 3674, 28338, 7, 621, 47, 186, 16750, 26866, 456, 3827, 179236, 33233, 4567, 225495, 4552, 19732, 8110, 43257, 4271, 81604, 48752, 25469, 191619, 831, 26171, 44389, 56, 82, 144, 40226, 1636, 43967, 42564, 42,...
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2932b390acc4aefae052f5481f73d6ead0759891
subsection
7
8
Conclusions
If we assume that multi-tiers exponential profiles are formed by secular evolution of galactic disks, the best place to search for them would be lenticular galaxies. Lenticulars galaxies had to reform secularly their stellar disks during their transformation from S to S0; hence S0s must be the hosts of both multi-tiers...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1317, "openalex_id": "", "raw": "Erwin, P., Pohlen, M., Beckman, J.E., Gutiérrez, L., Aladro, R. 2008, in: J.H. Knapen, T.J. Mahoney, & A. Vazdekis (eds.), Pathways through an Eclectic Universe. ASP Conf. Ser. v. 390 (San Francisc...
10.1017/S1743921308027567
0807.1817
Exponential bulges and antitruncated disks in lenticular galaxies
[ "Olga K. Sil'chenko" ]
[ "astro-ph" ]
2,008
en
Physics
[ 41591, 6024, 118, 1314, 78643, 80973, 60641, 7, 100, 4806, 40, 25667, 28, 137089, 22703, 49086, 28338, 2965, 3687, 33938, 2856, 2806, 121469, 5134, 18226, 1902, 17690, 29486, 320, 167201, 159, 47, 2389, 8110, 27980, 15044, 74189, 8516, 3684...
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2b2168fa9fdbe9e1a9da5bae37db136f430404b3
abstract
0
14
Abstract
The statistical properties of the return intervals $\tau_q$ between successive 1-min volatilities of 30 liquid Chinese stocks exceeding a certain threshold $q$ are carefully studied. The Kolmogorov-Smirnov (KS) test shows that 12 stocks exhibit scaling behaviors in the distributions of $\tau_q$ for different thresholds...
{ "cite_spans": [] }
10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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48f6fd7f4cc0756840a49bf617c624e011885af0
subsection
1
14
Introduction
In recent years many concepts and methods from statistical physics have been applied to the study of financial markets . The statistical analysis of the waiting time between two successive events has drawn much attention. Different definitions of event refer to a variety of variables characterizing the properties of st...
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10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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e8c4951afdb3aed71433a04bd7cde0772c58384a
subsection
2
14
Introduction
In addition, Lee et al. investigated the return intervals of 1-min volatility data of the Korean KOSPI index . They found that the interval return distribution had a power-law tail and no scaling was observed. However, it seems that they did not remove the intraday pattern from the intraday volatility series, which wea...
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10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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1319316bcdf92179ea777721b29676998de720b9
subsection
3
14
Preprosessing the data sets
Our analysis is based on the high-frequency intraday data of 30 most liquid stocks traded on the Shanghai Stock Exchange and the Shenzhen Stock Exchange. These 30 stocks are most actively traded stocks representative in a variety of industry sectors, and thus have the largest sizes among all the stocks. The basic infor...
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10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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1cbb9fbda2bf0b46215006238402c34336cba297
subsection
4
14
Preprosessing the data sets
When the threshold q is very small, say less than the minimum of r(t), then all \tau _q values equal to 1. [Figure: Illustration of volatility return intervals for stock000625, where \tau _2, \tau _3 and \tau _4 correspond to returnintervals for q=2, 3 and 4.]
{ "cite_spans": [] }
10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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subsection
5
14
Scaling and nonscaling behaviors of return interval distributions
Several empirical studies show that the probability distribution function (PDF) of the return intervals obeys a scaling form:P_q(\tau )=\frac{1}{\bar{\tau }} f \left( \frac{\tau }{\bar{\tau }} \right),where \bar{\tau } is the mean return interval which depends on the threshold q. The scaling form could be approximated ...
{ "cite_spans": [] }
10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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c22a272147fb3ad7835aba47aaaea3a7e9dbad1b
subsection
6
14
Complementary cumulative distributions
To make the observation of this possible scaling behavior (REF ) more clear, we study the complementary cumulative distribution function (CCDF) of the scaled return intervalsC_q(\tau /\bar{\tau })= \int _\tau ^\infty P_q(\tau )d\tau =\int _{\tau /\bar{\tau }}^\infty f(x)dx.If the PDFs for different q obey the scaling f...
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10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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95323d18a4dc8821dee290eae5067166b5c45129
subsection
7
14
Kolmogorov-Smirnov test of scaling in return interval distributions
The eyeballing of complementary cumulative distributions offers a qualitative way of distinguishing scaling and nonscaling behaviors. Here we further adopt a quantitative approach, the Kolmogorov-Smirnov (KS) test. We use the KS test to compare two distributions for q=2 and q=5, which behave most differently among all ...
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10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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8ea9c0aa91cc208c59ffc82af6ca0fd23e31ad5b
subsection
8
14
Kolmogorov-Smirnov test of the scaling function
We have demonstrated that the return distributions of 12 stocks show scaling behaviors. To further study the particular form of the scaling function, we perform the KS goodness-of-fit test , . Empirical studies have shown that the scaling form could be approximated by a stretched exponential function as in Eq. (REF ). ...
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10.1016/j.physa.2008.12.005
0807.1818
Statistical properties of volatility return intervals of Chinese stocks
[ "Fei Ren", "Liang Guo", "Wei-Xing Zhou" ]
[ "q-fin.ST", "physics.data-an", "physics.soc-ph" ]
2,008
en
Quantitative Finance
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