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95a11529d1c381eb6606e6b79c457898e3bb8e05
subsection
84
108
Conclusion
After defining adaptive convolutions (for other types of adaptive convolutions see Appendix ) and analyzing their theoretical properties, we have derived a formula for the adaptation function \mu _f, which allows automatic adjustment of the local smoothing of a function f. The requirements for such a formula were reaso...
{ "cite_spans": [ { "arxiv_id": "", "doi": "10.48550/arxiv.1805.01729", "end": 2192, "openalex_id": "https://openalex.org/W2802336905", "raw": "I. Klebanov. Axiomatic approach to variable kernel density estimation. ArXiv e-prints, 2018.", "source_ref_id": "5122feebb607cdd56ab37...
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ 0.018886689096689224, 0.01844426989555359, -0.03545449301600456, -0.012494505383074284, 0.025706034153699875, -0.014340458437800407, -0.008772089146077633, -0.026560358703136444, 0.062121644616127014, 0.042045000940561295, -0.020366501063108444, 0.025004267692565918, -0.015835527330636978, ...
3a9dbefd64de9cb50e49c3a8aa6514302b2ec77c
subsection
85
108
Other Types of Adaptive Convolutions
In the case of the common convolution f\ast g, the contribution of f(y) to (f\ast g) (x) depends, roughly speaking, on the distance between x and y. In the following, we will introduce two further types of adaptive convolutions, for which the contribution of f(y) to the convolution evaluated in x depends on the distanc...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.01740972138941288, -0.0380847193300724, -0.018493061885237694, 0.00703407684341073, 0.006965414620935917, -0.03494150936603546, -0.03210346773266792, -0.00647333450615406, 0.035887524485588074, -0.01747075468301773, -0.07421638071537018, -0.008620940148830414, -0.004001489374786615, 0.0...
bd7b455d07153f8115a02a2965bacadce6fb5c96
subsection
86
108
Other Types of Adaptive Convolutions
\end{} \end{align*}}\begin{}[Young^{\prime }s inequality] Under the conditions of Definition \ref {def\mathrel {\mathop }weightedAdapt}, we have\mathrel {\mathop } \left\Vert f\ast ^p [g\, |\, h]\right\Vert _p\le \left\Vert f\right\Vert _1\left\Vert g\right\Vert _p \qquad \text{and}\qquad \left\Vert f\ast ^p [g_1,g_2...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.016754046082496643, -0.037078626453876495, -0.018081553280353546, -0.037353284657001495, -0.006061516236513853, -0.02659590356051922, -0.007739972788840532, 0.05572475120425224, 0.04052709415555, 0.026244955137372017, -0.02664167992770672, -0.009170475415885448, -0.007492018863558769, 0...
b5b95131f48f34b79a707f20cc7ec746d95762a3
subsection
87
108
Other Types of Adaptive Convolutions
Let f\in L^q\left(\mathbb {R}^d\right), g_1=g_2=\mathrel {\mathop }g\in L^1\cap L^p\left(\mathbb {R}^n\right) and h\colon \mathbb {R}^d\rightarrow \mathbb {R}^n be a measurable function such that0 < \left\Vert g(h({\cdot )-z)_p < \infty for almost all z\in \mathbb {R}^d. Then \tilde{G}_p is symmetric and \left\Vert f\...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.035248056054115295, 0.018356453627347946, 0.01188668143004179, -0.029434414580464363, 0.0064468844793736935, -0.01976027339696884, -0.026230046525597572, 0.00875097792595625, 0.038696564733982086, 0.0035362497437745333, -0.05172766372561455, -0.019226212054491043, 0.001713764970190823, ...
d4211e7d6ff0561a3601904ee03811753053dcbc
subsection
88
108
Other Types of Adaptive Convolutions
\item If g_1\in L^1\left(\mathbb {R}^d\times \mathbb {R}^n\right),\ g_2,\, g\in L^p\left(\mathbb {R}^d\times \mathbb {R}^n\right) depend on an additional parameter in \mathbb {R}^d and \begin{} \item \displaystyle \int _{\mathbb {R}^d} |g_1(y,z-h(y))|\, \mathrm {d}y\le \Gamma _1 for some constant \Gamma _1>0 (independe...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.03345469385385513, 0.017292048782110214, -0.007631089072674513, -0.009722007438540459, -0.004075001459568739, -0.0006686741835437715, 0.006471163593232632, 0.02269485965371132, 0.04114683344960213, 0.01467458438128233, -0.05399758741259575, -0.045969683676958084, -0.00911152083426714, 0...
a3fba8520a729c929f1f35dfa0ac7079c0b49635
subsection
89
108
Other Types of Adaptive Convolutions
More precisely, in this case the linearization of h at y, h(x)-h(y)\approx Dh(y)\, (x-y), is meaningful and yields \begin{align*} G_p(x,y) &= \left\Vert g\right\Vert _p \frac{g\left(h(x)-h(y)\right)}{\left\Vert g(h({\cdot )-h(y))_p} \approx \left\Vert g\right\Vert _p \frac{g\left(Dh(y)\, (x-y)\right)}{\left\Vert g(Dh(y...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.01635691523551941, -0.019698485732078552, -0.006397048942744732, -0.02656472846865654, -0.008903227746486664, -0.014289412647485733, -0.02654946967959404, 0.00981872621923685, 0.04626321420073509, -0.00469193235039711, -0.029082350432872772, -0.01888979598879814, 0.008964261040091515, 0...
226de2d4a08fcae3172e0ed3dd36513b7f6707c6
subsection
90
108
Other Types of Adaptive Convolutions
For example, we can `let a value f(y) contribute strongly to f\ast ^p[g\, |\, h](x), even though x is far away from y (without contributing strongly to most values in between)^{\prime } by choosing h such that h(y)\approx h(x), see Figure \ref {fig\mathrel {\mathop }weighted_quadratic}. } \section {Proofs} \right.\beg...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.01829780451953411, 0.003637813962996006, 0.006733866408467293, -0.03394021466374397, -0.021807808429002762, -0.03610726073384285, 0.04379874840378761, 0.05423719435930252, 0.02537885680794716, 0.010179012082517147, -0.05036092922091484, 0.014574147760868073, -0.03772491589188576, -0.006...
68528f798fed6fdf9d89ab1ef3ad07f963ce8e3c
subsection
91
108
Other Types of Adaptive Convolutions
Hölder^{\prime }s inequality yields \begin{align*} |f \bar{\ast }G|(x) &\le \int _{\mathbb {R}^d} |f(y)|^{\frac{1}{p^{\prime }}}\, |f(y)|^{\frac{1}{p}}\, |G(x,y)|\, \mathrm {d}y \le \left\Vert |f|^{\frac{1}{p^{\prime }}}\right\Vert _{p^{\prime }}\, \left\Vert |f|^{\frac{1}{p}}\, |G(x,{\cdot )|_{p}, } which implies \beg...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.007306648883968592, 0.01929108053445816, -0.019489485770463943, -0.029241858050227165, -0.019809985533356667, -0.002937921555712819, 0.007165476214140654, 0.03708649054169655, 0.029714977368712425, -0.014071499928832054, -0.0776527002453804, -0.0002345329412491992, -0.028326142579317093, ...
9a43c4c5bb400915f88be7d3023f8fd06704e1cc
subsection
92
108
Other Types of Adaptive Convolutions
\end{align*}\end{}}\right.}\end{align*}\begin{}[Proof of Corollary \ref {cor\mathrel {\mathop }young}] First note that for p<\infty and y\in \mathbb {R}^d the change of variables formula implies\mathrel {\mathop } \begin{equation} \left\Vert g_{\mu ,p}({\cdot ,y)_p^p = \int _{\mathbb {R}^d}|\det \mu (y)|\, \left| g\bi...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.06435072422027588, -0.005735243204981089, -0.0025356414262205362, -0.034434352070093155, -0.03452593460679054, -0.011737596243619919, -0.012867092154920101, 0.044660866260528564, 0.005510107148438692, -0.018835103139281273, -0.0012134446296840906, -0.01438580546528101, -0.0032034174073487...
f6425b443202784f7f3140c0794eb58eedd4a35b
subsection
93
108
Other Types of Adaptive Convolutions
Since \frac{r-q}{qr} + \frac{r-p}{pr} + \frac{1}{r} = \frac{1}{q} - \frac{1}{r} + \frac{1}{p} - \frac{1}{r} + \frac{1}{r} = \frac{1}{q} + \frac{1}{p} - \frac{1}{r} = 1, the generalized Hölder's inequality yields |f \bar{\ast }G|(x) &\le \int _{\mathbb {R}^d} |f(y)|^{1-\frac{q}{r}}\, |f(y)|^{\frac{q}{r}}\, |G(x,y)|^{...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.051741477102041245, 0.021093428134918213, -0.019597657024860382, -0.01784241572022438, 0.0030297001358121634, 0.0026710203383117914, -0.0007268990739248693, 0.02225341461598873, 0.01205774862319231, -0.006643209140747786, -0.055099330842494965, 0.004208764992654324, -0.025244956836104393,...
39483bd60a4f51f32d981b8dd28df56ff03072db
subsection
94
108
Other Types of Adaptive Convolutions
\end{align*} \right. }\right.} [Proof of Proposition REF ] For all j=1,\dots ,d and \alpha \in \mathbb {N}^d with |\alpha |<m, we have by induction: \partial _{x_j}\partial ^\alpha \left(f\ast _{\mu }^p g\right)(x) &= \partial _{x_j}\left(\int _{\mathbb {R}^d} f(y)\, |\det (\mu (y))|^{1/p}\, \alpha (\mu (y))\, D^{|\al...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.00034682522527873516, 0.007345543708652258, -0.03786425665020943, -0.026697199791669846, -0.013668966479599476, 0.009328764863312244, 0.013821521773934364, 0.006102217361330986, 0.0364302359521389, 0.0036250983830541372, -0.018474461510777473, -0.0026906963903456926, -0.006914574652910232...
bbad90835d89d0fdce538a2533996289341c10fa
subsection
95
108
Other Types of Adaptive Convolutions
The observations \begin{} \begin{align*} \left({\rm tr}\left[\mu _t^{-1}(y)\partial _{k}\mu _t(y)\right] \right)_{k=1}^d j_t(y) &= \sum _{k=1}^d {\rm tr}\left[\mu _t^{-1}(y)\partial _{k}\mu _t(y)\right]\, j_{k,t}(y) = {\rm tr}\left[\mu _t^{-1}(y)\sum _{k=1}^d\partial _{k}\mu _t(y)\, j_{k,t}(y)\right] \\ &= {\rm tr}\lef...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ 0.00036994070978835225, 0.028954533860087395, -0.03228018805384636, -0.01919114962220192, -0.014095884747803211, 0.010213414207100868, 0.02962576597929001, 0.02478983998298645, 0.02382875792682171, 0.046559132635593414, -0.02880198135972023, 0.003932049963623285, -0.003943491727113724, -0....
60376110a7b368d2e22e7b5962d74a7509cdf6c8
subsection
96
108
Other Types of Adaptive Convolutions
\end{pmatrix} lead to \begin{align*} &\left(\nabla _y\Big [\delta _t(y) \, g_{\mu _t}(x,y)\Big ]\right)^{\intercal }j_t(y) \\ &= \delta _t(y) \left( g_{\mu _t}(x,y) \left({\rm tr}\left[\mu _t^{-1}(y)\partial _{k}\mu _t(y)\right] \right)_{k=1}^d + (\nabla g)_{\mu _t}(x,y)^{\intercal } \left[M_t(x,y)-\mu _t(y)\right] \ri...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.0151362968608737, 0.012786508537828922, -0.005977463908493519, -0.03228669613599777, -0.017928577959537506, 0.038786761462688446, 0.013343438506126404, 0.02511526644229889, 0.0034064296633005142, 0.03222566470503807, -0.008926142938435078, 0.0026072729378938675, -0.008956659585237503, 0...
b826f881dbbbd42821b985193bb8729fecb2e868
subsection
97
108
Other Types of Adaptive Convolutions
\end{align*} Combining these two, we get\mathrel {\mathop } \begin{align*} \partial _t \rho _{g,t}(x) &= \int _{\mathbb {R}^d} \underbrace{\partial _t\rho _t(y)}_{= -\operatorname{div}j_t(y)} \delta _t(y) \, g_{\mu _t}(x,y) + \partial _t\Big [\delta _t(y) \, g_{\mu _t}(x,y)\Big ]\, \rho _t(y) \, \mathrm {d}y \\ &= \int...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.015744362026453018, 0.011442123912274837, 0.0023551704362034798, -0.017559845000505447, -0.002164468402042985, -0.008520567789673805, 0.00038569490425288677, 0.02915453165769577, -0.0009239514474757016, 0.01267024502158165, -0.002175910398364067, -0.010175861418247223, -0.0237996168434619...
298b43791b684b7502e826924071c94ded3f1872
subsection
98
108
Other Types of Adaptive Convolutions
We have: &(f({\cdot \, - a)\ast ^p_{\mu _{f({\cdot \, - a)}} g) (x) = \int f(y-a) \left|\det \left(\mu _{f}(y-a)\right)\right| g\left(\mu _{f}(y-a)(x-y)\right)\, \mathrm {d}y \\ & \hspace{28.45274pt} = \int f(y) \left|\det \left(\mu _{f}(y)\right)\right| g\left(\mu _{f}(y)(x-a-y)\right)\, \mathrm {d}y = (f\ast ^p_{\mu...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.005618390627205372, 0.003526274347677827, -0.021588657051324844, -0.05312487855553627, -0.010733299888670444, 0.009733966551721096, -0.01843045838177204, 0.019681531935930252, 0.02998000755906105, 0.006201970856636763, -0.030468231067061424, 0.03019360452890396, -0.010618872940540314, 0...
b34a42695bcb1e72de656777575eebdd654a8b2f
subsection
99
108
Other Types of Adaptive Convolutions
\end{align*} \right. }\right.\begin{}[Proof of Proposition \ref {prop\mathrel {\mathop }muFourier}] The proof is analogous to the one of Proposition \ref {prop\mathrel {\mathop }muWigner2}. \end{} \right.\begin{}[Proof of Proposition \ref {prop\mathrel {\mathop }muFBI}] The proof is analogous to the one of Proposition ...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ 0.044177960604429245, -0.00014349065895657986, -0.025017905980348587, -0.003083380637690425, -0.023324621841311455, -0.021188946440815926, 0.019160054624080658, 0.03499456122517586, 0.06748732924461365, 0.04579497128725052, -0.03325551003217697, -0.012043680995702744, 0.00414549745619297, ...
fa548c3472d374d80675a2b79490a1bdcef0e5d8
subsection
100
108
Other Types of Adaptive Convolutions
Then we have for x,y\in \mathbb {R}^d \big (\nabla \tilde{f}\nabla \tilde{f}^{\intercal } - \tilde{f}\, D^2 \tilde{f}\big )(x) = A^\intercal \, \big (\nabla f\nabla f^{\intercal } - f\, D^2 f\big )(Ax)\, A, \qquad G_{\mu _{\tilde{f}}^{-2}(x)}(y) = *{\det A}\, G_{\mu _f^{-2}(Ax)}(Ay), and, since for any functions \phi...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ 0.014687075279653072, 0.009872766211628914, 0.009514173492789268, -0.0009026829502545297, -0.006878129206597805, -0.002988915191963315, 0.008552837185561657, -0.010902768932282925, 0.07165767252445221, 0.024826880544424057, -0.033021122217178345, -0.024414878338575363, 0.0002694220165722072,...
5d47501f3997524c208c2f569aaf6f22b5ffe2a6
subsection
101
108
Other Types of Adaptive Convolutions
Therefore, \mu _{f^{(t)}}(x+a_k^{(t)}) \stackrel{(A1)}{=} \mu _{\tilde{f}^{(t)}}(x) \xrightarrow{} \mu _{f_k}(x). } }}}\begin{}[Proof of Proposition \ref {prop\mathrel {\mathop }muWigner2}] As the Wigner transform is real-valued, we get for real-valued functions~f\mathrel {\mathop } \begin{align*} W f(x,-\xi ) &= (2\...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.005172934383153915, -0.004856301937252283, -0.011620028875768185, -0.014893168583512306, -0.01591554842889309, 0.0057489764876663685, 0.015656137838959694, 0.03415052220225334, 0.046693746000528336, 0.026490308344364166, 0.0038415524177253246, 0.014999983832240105, 0.0035401794593781233, ...
c4f2879055e7d1aa9e4a2c54e89b5f62be36663a
subsection
102
108
Other Types of Adaptive Convolutions
For the covariance matrix, we use the transformation z_1 = y_1-y_2,\qquad z_2 = y_1+y_2 and the function F(z_1,z_2) = f\left(x+\frac{z_2 + z_1}{4}\right)f\left(x-\frac{z_2 + z_1}{4}\right)f\left(x+\frac{z_2 - z_1}{4}\right)f\left(x-\frac{z_2 - z_1}{4}\right) to compute\mathrel {\mathop } \begin{} \begin{align*} \in...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.005715889856219292, -0.0007206866866908967, 0.0014432811876758933, 0.03531793877482414, 0.008554755710065365, 0.0049985419027507305, 0.03183804079890251, 0.022527778521180153, -0.011828609742224216, 0.023825110867619514, -0.049848053604364395, -0.01061522401869297, 0.002384800463914871, ...
f61082c0e7230c28c36f0f7269e396092adb3bd3
subsection
103
108
Other Types of Adaptive Convolutions
\end{align*} \end{} Taking the quotient proves the formula for the covariance matrix. \end{} \right.}\end{} [Proof of Theorem REF ] Adaptation Axiom REF (A1) follows from \left(f({\cdot -a)\ast g({\cdot -b)(x) }}\right.&= \int f(y-a)\, g(x-y-b)\, \mathrm {d}y = \int f(y)\, g(x-(a+b)-y)\, \mathrm {d}y \\ &= (f\ast g)(x...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ 0.0013511285651475191, -0.00341167114675045, -0.029612313956022263, -0.011846451088786125, 0.0258440300822258, 0.0018088150536641479, 0.03987974673509598, 0.038262587040662766, 0.020611146464943886, -0.006117742508649826, -0.03551647067070007, 0.0018316993955522776, -0.021862156689167023, ...
808f065bd0107ec84bf7f7566d50afca8e425ce2
subsection
104
108
Other Types of Adaptive Convolutions
The claim follows from the definitions (REF ) of \mu _f^{(d)} and (REF ) of \mu _f^{(e)}. [Proof of Proposition ] For the h-adaptive convolution of type two the property \left\Vert G({\cdot ,y)_p = \left\Vert g\right\Vert _p is straightforward for all y\in \mathbb {R}^d, 1\le p \le \infty and Theorem \ref {theorem\mat...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.03579450771212578, 0.008384092710912228, -0.010909237898886204, -0.02456485852599144, -0.020018070936203003, -0.027677424252033234, 0.006740078330039978, 0.03478750213980675, 0.03912068158388138, 0.005679669789969921, -0.04543735831975937, -0.005008331965655088, -0.0037705532740801573, ...
352c3da9918e9b05a4830c8cb63059942206dc44
subsection
105
108
Other Types of Adaptive Convolutions
Hölder^{\prime }s inequality yields \begin{align*} |\tilde{G}(x,y)| &\le \left\Vert g_2\right\Vert _p \int |g_1(z-h(y))|^{1/p^{\prime }}\, |g_1(z-h(y))|^{1/p} \gamma (x,z)\, \mathrm {d}z \\ &\le \left\Vert g_2\right\Vert _p \left\Vert g_1({\cdot -h(y))^{1/p^{\prime }}_{p^{\prime }} \left\Vert g_1({\cdot -h(y))^{1/p}\, ...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.023305442184209824, 0.013987843878567219, -0.02129082754254341, -0.02271021530032158, -0.027670443058013916, 0.0026613534428179264, 0.020527714863419533, 0.03063131868839264, 0.01092776469886303, -0.008707108907401562, -0.049419138580560684, 0.00428105890750885, -0.03565259650349617, -0...
a9ab97aae47b9ffa68b1c631b988addfcda80539
subsection
106
108
Other Types of Adaptive Convolutions
\end{align*} \end{} Therefore \left\Vert \tilde{G}({\cdot ,y)_p \le \left\Vert g_1\right\Vert _1 \left\Vert g_2\right\Vert _p (for all y\in \mathbb {R}^d and 1\le p\le \infty ) also holds for type three and again Theorem \ref {theorem\mathrel {\mathop }young1} proves the claim. } \right.}\right.}\right.\begin{}[Proof o...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.05638016015291214, 0.000177927955519408, -0.012020445428788662, -0.038013894110918045, 0.006902603432536125, -0.01806117594242096, 0.015956073999404907, 0.005323776043951511, 0.008344141766428947, 0.0014034021878615022, -0.02501717023551464, -0.0007612885092385113, -0.008588211610913277, ...
30f0452c817821d01e4abbd5a1ce8442a0c9cd08
subsection
107
108
Other Types of Adaptive Convolutions
Springer, 1997. R. A. Horn and C. R. Johnson. Matrix analysis. Cambridge University Press, 2012. I. Klebanov. Axiomatic approach to variable kernel density estimation. ArXiv e-prints, 2018. W. Young. On the multiplication of successions of fourier constants. Proceedings of the Royal Society of London. Series A, Contai...
{ "cite_spans": [] }
1805.00703
Adaptive Convolutions
[ "Ilja Klebanov" ]
[ "math.FA" ]
2,018
en
Mathematics
[ -0.015388227999210358, -0.002168618608266115, -0.03720029816031456, 0.02011074312031269, -0.009040679782629013, -0.04476853087544441, 0.053679510951042175, -0.014373536221683025, 0.004844583570957184, 0.01570102758705616, -0.0059317536652088165, -0.00283236475661397, -0.022399522364139557, ...
77809e708c3379e7ab4537fa384e443523a2879d
abstract
0
51
Abstract
An analysis of the transmission of `scalar' phonons across partially unzipped square and triangular lattice tubes, assuming nearest neighbor interactions between particles, is presented. The phonon transport is assumed to involve the out-of-plane phonons in the unzipped portion and the radial phonons in the tubular por...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.01390131376683712, 0.003845368977636099, -0.058382466435432434, 0.013153603300452232, -0.008072222582995892, 0.02360629290342331, 0.02227872423827648, 0.014778729528188705, -0.011352993547916412, 0.02357577346265316, 0.0017805813113227487, 0.05813831463456154, -0.010986768640577793, 0.0...
6eee9c56247fec6b33d989409f972ddf22a06406
subsection
1
51
Introduction
The rise of nanostructures in technological applications has invigorated a slurry of questions concerning the nature of thermal transport , , . The reduced physical dimensions overcome the hurdles of the phonon mean free path, while new physical processes become crucial in the transport problem , . For instance, the th...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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e0ecb8e962a31326fff3fdddde8ec485475cee5e
subsection
2
51
Square lattice model
Consider a partly unzipped two-dimensional tube of square lattice, denoted by {{\mathfrak {S}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}}}, with {\mathtt {N}} number of rows containing infinite number of particles with unit mass, as shown schematically in Fig. REF (a). The `in-plane' nearest neighbors, ...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.04131584241986275, 0.01119860727339983, -0.04177355021238327, 0.00580527214333415, 0.03326016664505005, -0.004203291609883308, 0.01655379869043827, 0.00413463544100523, 0.004073607735335827, 0.05065310001373291, 0.0039134095422923565, 0.012342878617346287, -0.011564773507416248, -0.0090...
8e37f3e0e2f33315e316118969103f89646a9f7b
subsection
3
51
Square lattice model
The total displacement field {\mathtt {u}}^{{t}}, a sum of the incident wave field {\mathtt {u}}^{i} and the scattered wave field {\mathtt {u}}^{{s}}, of an arbitrary particle in the lattice {{\mathfrak {S}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}}} satisfies the discrete Helmholtz equation for all ({...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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b36c7814c6b027f5150cddcd8a42a9a892ae3ee0
subsection
4
51
Triangular lattice model
Similar to the square lattice, {\mathtt {N}} number of rows of particles with unit mass, are arranged in the form of one-dimensional lattices, but now these rows form a two-dimensional strip of triangular lattice {{\mathfrak {T}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}}}, as shown schematically in Fig...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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673e0539c7f735da3267dc79e2c2f47140b5de74
subsection
5
51
Triangular lattice model
Without any loss of generality, it is assumed that a(i)y=-a(i)N-y-1, yZ0N, as the definition of the incident wave mode on the replica {{\mathfrak {T}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}}}{{^\mathrm {R}}} in terms of that on {{\mathfrak {T}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ ...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.02380877546966076, 0.0075661540031433105, -0.03072247840464115, 0.008851980790495872, 0.03537739813327789, 0.006787790451198816, 0.002623162465170026, -0.016101447865366936, 0.007333408109843731, 0.04532824456691742, -0.010393446311354637, 0.026952754706144333, -0.03180608153343201, 0.0...
b8c3e70d2e4cd07c90aad4044b45efaf520b2f72
subsection
6
51
Wiener–Hopf formulation
The boundaries are such that {{\mathtt {y}}}=-1 and {{\mathtt {y}}}={{\mathtt {N}}}-1 are identified as same (shown schematically in Fig. REF ), while the unzipped portion lies along the broken bonds between {\mathtt {y}}=0 and {\mathtt {y}}=-1\simeq {{\mathtt {N}}}-1.
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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6f6e0a92e84693fec263a542dd44fb57a449c4a4
subsection
7
51
Square lattice tube
The equation of motion at {\mathtt {y}}=0, {\mathtt {y}}={\mathtt {N}}-1\simeq -1, is 2utx, y =utx+1, y+utx-1, y+utx, y1NH(x)+utx, y1 -(3+H(x))utx, y, xZ, where the letter {{\mathit {H}}} stands for the Heaviside function: {{\mathit {H}}}(m)=0, m<0 and {{\mathit {H}}}(m)=1, m\ge 0. Suppose the discrete Fourier trans...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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fd468d2a493b7cbac2850e528ad20f76fcb0483d
subsection
8
51
Square lattice tube
Introducing vx=ux, 0-ux, -1, vix=uix, 0-uix, -1, with {\mathrm {v}}^F={\mathtt {u}}^F_{0}-{\mathtt {u}}^F_{-1}, it is found that {\mathtt {u}}^F_{0}={{\mathrm {v}}}^F{{\mathtt {U}}_{{\mathtt {N}}-1}}/({{\mathtt {U}}_{{\mathtt {N}}-1}-{\mathtt {U}}_{{\mathtt {N}}-2}-1}), as well as in the context of (REF ), -{\mathtt ...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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75d8b778177f322e4c035ec7f8a016a59dd0b768
subsection
9
51
Square lattice tube
Finally, using (), for {{z}}\in {{{A}}}{{A}} is an annulus containing the unit circle {\mathbb {T}} in the complex plane that makes the Wiener–Hopf problem well-defined. v+(z)+L(z)v-(z)=(1-L(z))Av(i)D-(zzP-1), with v(i):=a(i)0-a(i)N-1, is obtained as a Wiener–Hopf equation, using (REF ), with the kernel \operatorna...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.04299670830368996, 0.034787971526384354, -0.04806232824921608, 0.021330518648028374, 0.007373371161520481, 0.002902811858803034, 0.03457435965538025, 0.00713687390089035, -0.023436106741428375, 0.012564864940941334, 0.002649149624630809, 0.01448735874146223, -0.04440043494105339, 0.0144...
9303d6c3772cac5a8449d2e3791d9814f1d2f569
subsection
10
51
Square lattice tube
Additionally, using the even/odd mode based factorizations given by , from (REF ),L= 2TN2(+1)UN-1, for {\mathtt {N}}=2{\mathrm {N}}VNWN, for {\mathtt {N}}=2{\mathrm {N}}+1.This completes the Wiener–Hopf formulation for {\mathfrak {S}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}} assuming incidence of wave...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.034035418182611465, 0.03534799441695213, -0.0011456429492682219, 0.006925368215888739, -0.008020454086363316, 0.029945064336061478, 0.04975581541657448, 0.015827232971787453, -0.017490847036242485, 0.03620269522070885, -0.0034111731220036745, 0.001903999364003539, -0.031043965369462967, ...
bfd2c4fc23dc7b4a27ce787c6a430fa67c27816a
subsection
11
51
Triangular lattice tube
In terms of a more convenient labelling shown in Fig. REF (b), it is required that {\mathtt {u}}^F_{{\mathrm {N}}}={\mathtt {u}}^F_{-{\mathrm {N}}}. Due to the manufactured symmetry on {\mathfrak {R}}{\mathbin {{{\circledcirc }\\{\circ }}}}, i.e., odd symmetry (REF ) in the choice of the incident wave mode (REF ), usin...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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e4b14b0b3eda74ca28b9d148c7214d3e2ba404ff
subsection
12
51
Triangular lattice tube
The details of aforementioned `even' and `odd' modes has been provided by .The Wiener–Hopf kernel (REF ) can be simplified to (compare with (REF )) L(z) =112(z+z-1)12(z+z-1)WN-WN-12(+1)UN-1=:ND, where {\vartheta }, the argument of the Chebyshev polynomials, is given by (REF ) using the definition of {{Q}} for triang...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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1ade62096ce9865e365570c46b736eada499637f
subsection
13
51
Triangular lattice tube
Indeed, {{N}}(-{z})=-{\frac{1}{2}}({z}+{z}^{-1})({{\mathtt {U}}}_{{\mathrm {N}}}({\vartheta }(-{z}))+{{\mathtt {U}}}_{{\mathrm {N}}-1}({\vartheta }(-{z})))-({{\mathtt {U}}}_{{\mathrm {N}}-1}({\vartheta }(-{z}))+{{\mathtt {U}}}_{{\mathrm {N}}-2}({\vartheta }(-{z})))=(-1)^{{\mathrm {N}}}({\frac{1}{2}}({z}+{z}^{-1}){{\mat...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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ec6185795cd67a9c0dd41593f183ac3de9f18ca2
subsection
14
51
Incidence from unzipped portion
In contrast to §REF and §REF discussed so far in this paper, consider the case when a wave mode is incident from the unzipped portion. The scattering of such a wave (Fig. REF ) occurs due to the `new' bonds placed between the `through-crack'. It is assumed that the incident wave has the form (REF ), with {}_x such that...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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d9525dbf30e3965fc4a6d889f20fa734b23efc33
subsection
15
51
Exact Solution of Wiener–Hopf equation
The multiplicative factors for the Wiener–Hopf kernels (REF ), and (REF ), can be constructed easily (see Appendix for the details). Using \operatorname{{L}}_{{}}=\operatorname{{L}}_{{}+}\operatorname{{L}}_{{}-}, Wiener–Hopf equations (REF ) and (REF ) (resp. (REF )), can be expressed as {{\operatorname{{L}}}_{{}+}^{-...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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b352ad34b80db4f439b2c150dcfad054e37fcdcc
subsection
16
51
Square lattice structure
Using (REF ) for {{\mathfrak {s}}}={{\mathcal {R}}} and (REF ) for {{\mathfrak {s}}}={{\mathcal {L}}},C(z)=(1L+(z)-L-(z))Av(i) (D-(z zP-1)s,R-D+(z zP-1)s,L), zA, , leading to C(z)=Av(i)(1L+(zP)-L1(z))D-(z zP-1)s,R Av(i)(L-(zP)-L1(z))D+(z zP-1)s,R, zA. Note that {{{\mathrm {v}}}_{({{{\kappa }}^{i}})}} denotes the ex...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
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0bea6041d6785560f2d2a69233b8791f89fefb91
subsection
17
51
Square lattice structure
Thus, it is required that ahead and behind the edge of unzipped portion ux, yAa=1NRAaa(a)yzax, x+, ux, y-Aa(a)yzax+Ab=1NLAba(b)yzbx, x-. Comparing (REF ) with the expression of {\mathtt {v}} ({\mathtt {v}}_{{\mathtt {x}}}={\mathtt {u}}_{{\mathtt {x}}, 0}-{\mathtt {u}}_{{\mathtt {x}}, -1}) based on (REF ), the coeffi...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.07651860266923904, -0.006044756155461073, -0.04582573473453522, -0.03508628159761429, 0.028511416167020798, -0.002183358184993267, 0.026467259973287582, 0.0218755342066288, -0.003739358624443412, 0.0447273813188076, 0.004984539933502674, 0.005133275408297777, -0.015232021920382977, 0.03...
52db579aa86af445d1a68873a1e8ef476f65d919
subsection
18
51
Square lattice structure
(REF ), and the numerical solution on a finite grid is shown in the same figures in (c), (d), and (e), where the displacement of particles located at lattice sites forming a discrete rectangle (shown as white bubbles in top of part (a)) with two sides aligned with `boundary' of the strips is plotted. Note that the far ...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.05307380482554436, -0.006863123271614313, -0.042422421276569366, -0.021119650453329086, 0.0038531154859811068, -0.032808706164360046, 0.02345440909266472, 0.021455368027091026, -0.018662812188267708, 0.03985876217484474, -0.00962897390127182, 0.02786451019346714, -0.013726246543228626, ...
500960afb97726244f6140976fa52b6d8940f3b0
subsection
19
51
Square lattice structure
The expression for the reflectance and the transmittance (using the far-field expansion (REF ) for a wave incident from the tubular portion) is given by.\hspace{-32.52127pt} {{R}}_{{{\mathcal {L}}}\leftarrow {{\mathcal {R}}}}&=&\frac{-{{\mathtt {V}_g}}({}_{\tilde{{\mathsf {a}}}})^{-1}}{|{\operatorname{{L}}}_{{}+}({{z}}...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.042493004351854324, -0.02248282916843891, -0.01863647811114788, 0.006536504719406366, 0.03357924148440361, -0.012264054268598557, 0.003371279453858733, 0.031076060608029366, 0.0016112312441691756, 0.037395063787698746, -0.006998219061642885, 0.05467310920357704, -0.02980920858681202, 0....
c4675fe675ecaeeca82fa805c7ddc99b8ec5ca4b
subsection
20
51
Square lattice structure
And for the unzipped portion, {{{\mathrm {v}}}_{({{\mathsf {b}}})}}=2/\sqrt{{\mathtt {N}}}\cos {{\frac{1}{2}}}{{}} for an appropriate {} . After various manipulations, analagous to those applied for the bifurcated waveguides of square lattice , it is found that the reflectance {{R}}_{{{\mathcal {L}}}\leftarrow {{\mathc...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.06709542125463486, 0.017033323645591736, -0.04240015521645546, 0.005326729267835617, 0.0338224433362484, -0.01562914252281189, -0.0118744857609272, 0.005788430105894804, -0.01819329895079136, 0.03434137627482414, 0.019124330952763557, 0.037149738520383835, -0.016468599438667297, 0.01909...
420a1f37af7746171443d59f038578c7c079edf9
subsection
21
51
Square lattice structure
N in the plot label refers to N_{\text{grid}}.][Figure: Illustration for triangular lattice structure with details same as those in Fig. except for the incidence from the unzipped side.]
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.08690264821052551, 0.040308427065610886, -0.04500751569867134, 0.009024388156831264, -0.016492584720253944, -0.05260539427399635, -0.00033660282497294247, 0.03957609832286835, -0.027980944141745567, 0.03557882085442543, -0.008452259004116058, 0.00609127152711153, -0.012739415280520916, ...
e23451f9bb3f5fc10914d9907906fd1e25ce2533
subsection
22
51
Triangular lattice structure
Using (REF ) for {{\mathfrak {s}}}={{\mathcal {R}}} and (REF ) for {{\mathfrak {s}}}={{\mathcal {L}}}, in the context of the first paragraph of this section §,The odd symmetry of the incident wave on {{\mathfrak {T}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}}} is assumed (i.e., - sign in (REF )) since t...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.05937743932008743, 0.04372449591755867, -0.03591328114271164, -0.0037244390696287155, -0.00035709229996427894, 0.010511576198041439, 0.04164964333176613, -0.006083441432565451, -0.011426953598856926, 0.004664607346057892, 0.006289401091635227, 0.030146406963467598, -0.04177169129252434, ...
83e170aedb9def9f83cef03d19d620514801c71c
subsection
23
51
Triangular lattice structure
Note that \sum \nolimits _{{\mathtt {x}}\in {\mathbb {Z}}}({\mathtt {u}}_{{\mathtt {x}}, 0}-{\mathtt {u}}_{{\mathtt {x}}-1, -1}){{z}}^{-{\mathtt {x}}} =(1+{{z}}^{-1}){\mathtt {u}}_{{0}}^F({{z}}), and therefore, using (REF ), (1+z-1)u0;(z)u-1, 0=v. Note that the Fourier transform of the second type of slant bondlengt...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.05260905623435974, 0.004466734826564789, -0.05285318195819855, -0.012068957090377808, 0.018217869102954865, 0.036252643913030624, 0.01640218496322632, 0.029157744720578194, -0.028349079191684723, 0.04150134325027466, -0.0026911026798188686, 0.051510490477085114, -0.02079644612967968, 0....
e55aec56b770eff1d3c774cc3366fe261569ea2b
subsection
24
51
Triangular lattice structure
As a result the following asymptotic expression holds, vx Aa(a)0(1+za-1)D+(za)N+(za)a=1NR 1za-zaN+(za)D'+(za)zax,vxAa(a)0(1+za-1)(-zax +D+(za)N+(za)b=1NL 1zb-zaD-(zb)N'-(zb)zbx), as {\mathtt {x}}\rightarrow \pm \infty , respectively, where the values of {z}, corresponding to the outgoing wave modes, that appear in t...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.06062065064907074, 0.011440737172961235, -0.07328173518180847, -0.0048890081234276295, 0.009892423637211323, 0.010678021237254143, 0.056624021381139755, 0.012569556012749672, -0.007978007197380066, 0.02361368015408516, 0.004347479902207851, 0.02520012855529785, -0.016413643956184387, 0....
27633d30434b42b793d778e056a8ca86756c5cb8
subsection
25
51
Triangular lattice structure
Further, on the lattice {\mathfrak {T}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}} where {\mathtt {x}}\in 2{\mathbb {Z}} at {\mathtt {y}}=0, the total displacement field in the far-field is asymptotically given by (with {{a}}_{({{{\kappa }}^{i}})}={{a}}_{(\tilde{{\mathsf {a}}})}\delta _{{{\mathfrak {s}}...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.059842389076948166, 0.006812755484133959, -0.03591763973236084, -0.0053899348713457584, 0.029905935749411583, -0.001369417179375887, 0.03472750633955002, 0.02755618467926979, -0.025359012186527252, 0.03814532607793808, 0.0032900343649089336, 0.006007888820022345, -0.030729874968528748, ...
40cb224ff245348dfa5222692e79c704c93b3f06
subsection
26
51
Triangular lattice structure
(REF ), and the numerical solution on a finite grid is shown in the same figures in (c), (d), and (e), where the displacement of particles located at lattice sites forming a discrete rectangle (big white dots) with two sides aligned with `boundary' of the strips is plotted. Note that the far field displacement, for any...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.07535570859909058, 0.003483676118776202, -0.03246092051267624, -0.03905073180794716, 0.004580071195960045, -0.011745727621018887, 0.018442317843437195, 0.013019452802836895, -0.022057561203837395, 0.04210156947374344, -0.015155039727687836, 0.006708031054586172, -0.01414826326072216, 0....
688ba0ec276fd80b27cb5121f699a363b9ee9b30
subsection
27
51
Triangular lattice structure
The dispersion relations for the odd modes in the portion ahead of the unzipped portion and behind are almost overlapping.Using (REF ), for incidence from the tubular portion, the reflectance and the transmittance, respectively, are given by\hspace{-54.2025pt}&&{{R}}_{{{\mathcal {L}}}\leftarrow {{\mathcal {R}}}}=\hspac...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.053021397441625595, -0.00426337169483304, -0.02022622898221016, -0.013064679689705372, -0.007500941399484873, 0.02399386093020439, 0.005312054418027401, 0.01796870119869709, -0.003399638691917062, 0.01812123693525791, -0.035967908799648285, 0.01967710070312023, -0.02434469200670719, 0.0...
5be4d957bbf04c5032c1731f5767ef9e346b2459
subsection
28
51
Triangular lattice structure
The expression {\mathtt {V}_g}({}) denotes the group velocity of the propagating wave with wave number {} in the appropriate lattice strip. [Figure: Choice of {}_{\tilde{{\mathsf {a}}}} ({}_{\tilde{{\mathsf {b}}}}), so that the group velocity is positive (resp. negative), for wave incident from the tubular (resp. unzip...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.050475019961595535, -0.0014676741557195783, -0.03131038323044777, 0.004978076089173555, 0.011947382241487503, -0.02537483721971512, 0.026381896808743477, 0.04540921002626419, -0.0010003835195675492, 0.03146296739578247, -0.011367560364305973, 0.007888629101216793, 0.0025672377087175846, ...
a7efaa70020a14c31a636bdefae286c795582095
subsection
29
51
Triangular lattice structure
On the other hand, (while observing that {z}\ne \pm 1, {{N}}({z})=0, using (REF )) it is found that {{N}}^{\prime }({{z}})={\frac{1}{2}}{z}^{-1}({z}-{z}^{-1}){{\mathtt {W}}}_{{\mathrm {N}}}+({\vartheta }-1)^{-1}{\vartheta }^{\prime }(\cos {}({\mathrm {N}}+{\frac{1}{2}})(1-\alpha ){\mathtt {U}}_{{\mathrm {N}}}-({\mathrm...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.041247088462114334, 0.029120078310370445, -0.031637005507946014, -0.009549067355692387, 0.000844219175633043, -0.0014033772749826312, 0.07913827896118164, 0.03639628365635872, -0.02144726552069187, 0.04115556553006172, -0.008740600198507309, -0.008687210269272327, -0.014941392466425896, ...
296a6cfb8b52bcaab57705dda3d6a331207ab736
subsection
30
51
Triangular lattice structure
Then, (REF ) implies\hspace{-25.29494pt}{{R}}_{{{\mathcal {L}}}\leftarrow {{\mathcal {R}}}} &=&-\frac{{\mathtt {V}_g}({}_{\tilde{{\mathsf {a}}}})^{-1}}{|{\operatorname{{L}}}_{{}+}({{z}}_{\tilde{{\mathsf {a}}}})|^2{\mathrm {N}}}\sum \limits _{{\mathsf {a}}=1}^{N^{{{\mathcal {R}}}}}\frac{\cos ^2{\frac{1}{2}}{}_{\tilde{{\...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.04765164852142334, 0.04169900715351105, -0.003445663023740053, 0.017903709784150124, -0.012553965672850609, 0.02703109197318554, 0.00854738149791956, 0.024558456614613533, -0.004342374857515097, -0.0034094129223376513, -0.030190570279955864, 0.03712005540728569, -0.005021586548537016, 0...
0b6795e646acc16abbdb96f1cb0490f434a8c5da
subsection
31
51
Triangular lattice structure
Also the identity {{\mathtt {U}}}_{n}^2=1+{{\mathtt {U}}}_{n-1}{{\mathtt {U}}}_{n+1} implies {{\mathtt {U}}}_{{\mathtt {N}}}^2=1 when {{\mathtt {U}}}_{{\mathtt {N}}-1}=0, so that {{\mathtt {T}}}_{{\mathtt {N}}}={{\mathtt {U}}}_{{\mathtt {N}}}=\pm 1. But {{\mathtt {T}}}_{{\mathtt {N}}}\ne 1 when {{D}}\ne 0 which leaves ...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.02626298926770687, 0.040531374514102936, -0.031985603272914886, 0.038364410400390625, -0.022264787927269936, -0.036136407405138016, 0.02777375839650631, 0.043736040592193604, -0.027376990765333176, 0.007519516162574291, -0.0017463513650000095, -0.017839299514889717, -0.01072799600660801, ...
99317e5f4fd263f52c9852327d4d96128acc5de9
subsection
32
51
Triangular lattice structure
Finally, the expected, and elegant, form of the expression (REF ) results.Similarly, (using (1+\alpha ^2-2{\vartheta }\alpha ){\mathtt {U}}^2_{{\mathrm {N}}}=1) it is found that{{T}}_{{{\mathcal {L}}}\leftarrow {{\mathcal {R}}}}&=&{2}i\frac{\sin ^2{\frac{1}{2}}{{}_{\tilde{{\mathsf {a}}}}}\cos ^2{\frac{1}{2}}{}_{\tilde{...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.025082040578126907, 0.06401717662811279, -0.027401061728596687, 0.006899849511682987, 0.0042680660262703896, -0.016080578789114952, 0.008536132052540779, 0.04708222299814224, 0.016095835715532303, 0.026622969657182693, 0.0009134958381764591, 0.04775352030992508, 0.007231683470308781, 0....
81da55f1e8e7b40f175daf5a9a4c7e11230fb480
subsection
33
51
Triangular lattice structure
In fact, by inspection it is clear that the relations (REF ) and (REF ) are same as those for the square lattice structure; moreover, for the incidence from the unzipped portion, the expressions retains the same form (recall (REF ) and statement preceding it).It is worth a non-trivial note that the final expression for...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.0020453196484595537, 0.03072558529675007, -0.012477976270020008, 0.03876949101686478, 0.019476326182484627, -0.021964291110634804, 0.06245856732130051, 0.04597390070557594, -0.008181278593838215, 0.020163187757134438, 0.019323691725730896, 0.004972110968083143, -0.04331803694367409, -0....
6de095f564075328bdcf738bd6dca332e492fcdb
subsection
34
51
Triangular lattice structure
In particular, with {{z}}_{{P}}={{z}}_{\tilde{{\mathsf {a}}}}\delta _{{{\mathfrak {s}}}, {{\mathcal {R}}}}+{{z}}_{\tilde{{\mathsf {b}}}}\delta _{{{\mathfrak {s}}}, {{\mathcal {L}}}}, in the first two equations,\hspace{-25.29494pt}{{R}}\delta _{{{\mathfrak {s}}}, {{\mathcal {R}}}}+{{T}}\delta _{{{\mathfrak {s}}}, {{\mat...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.04839480295777321, 0.037745505571365356, -0.03704369068145752, 0.0023533727508038282, -0.023571869358420372, -0.0035262450110167265, 0.03951530158519745, -0.0004364896158222109, 0.001499941456131637, 0.02451779693365097, -0.008612505160272121, 0.031368132680654526, -0.024197401478886604, ...
e1cc384374ef7472c3b151767674a3786604f09b
subsection
35
51
Triangular lattice structure
REF with {}_{\tilde{{\mathsf {a}}}} and {}_{\tilde{{\mathsf {b}}}}, respectively, as a variable on horizontal axis. [Figure: Reflectance for the partly unzipped tube with (a) {\mathtt {N}}=6 (b) {\mathtt {N}}=8. The critical point associated with local maximum of the dispersion curves in the interval (0, {\frac{1}{2}}\...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.08017876744270325, 0.012951250188052654, -0.026527944952249527, 0.006124767009168863, 0.0005949337501078844, -0.014804697595536709, -0.0016846922226250172, 0.020975228399038315, -0.011250349693000317, 0.031577255576848984, -0.002715338720008731, 0.015727607533335686, -0.002627624198794365...
7efea196d896ccf4dc888b454e8aa3c8b6d5f952
subsection
36
51
Scattering matrix
Under the limit {}_2=\Im {}\rightarrow 0 and |{\mathtt {x}}|\rightarrow \infty , it is easy to see that the far-field can be determined (suitably) in terms of the propagating waves associated with the two different portions of the lattice strip. Suppose that the symbol {\mathbb {T}} denotes the unit circle (as a counte...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.07355855405330658, 0.007600033655762672, -0.029896516352891922, 0.0398009791970253, 0.02354789525270462, -0.020282017067074776, 0.012399652972817421, 0.0061197057366371155, -0.022861145436763763, 0.04071664437651634, -0.008096019737422466, 0.014215725474059582, -0.01845068298280239, 0.0...
339bf56846c56ebc3a704568a03770466d337695
subsection
37
51
Scattering matrix
Thus, () and () can be written as, respectively, {{\mathcal {Z}}}^+_{{{\mathcal {R}}}}=\lbrace {z}_{{\mathsf {a}}}\rbrace _{{\mathsf {a}}=1}^{N^{{{\mathcal {R}}}}}, {{\mathcal {Z}}}^{-}_{{{\mathcal {L}}}}=\lbrace {z}_{{\mathsf {b}}}\rbrace _{{\mathsf {b}}=1}^{N^{{{\mathcal {L}}}}}, and {{\mathcal {Z}}}^{-}_{{{\mathcal ...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.03130219876766205, 0.026466527953743935, -0.0385938435792923, 0.024056319147348404, 0.020868131890892982, -0.015651099383831024, 0.002450251253321767, 0.023019013926386833, -0.03276662901043892, 0.06449595093727112, 0.025673294439911842, 0.03197339549660683, -0.02384275756776333, 0.0088...
890396b85e6353737caf036709be6ac634ffc771
subsection
38
51
Scattering matrix
The asymptotic form of solution to equation of motion is thus u{{ll} \widetilde{{\mathsf {I}}}_{{{\mathcal {R}}}}{\mathtt {u}}_{{\tilde{{\mathsf {a}}}}}+\widetilde{{\mathsf {I}}}_{{{\mathcal {R}}}}\sum \limits _{{{\mathsf {a}}}=1}^{N^{{{\mathcal {R}}}}}{{\tau }}^{{{\mathcal {R}}}\tilde{{{\mathcal {R}}}}}_{{\mathsf {a}...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.028119882568717003, 0.01750054582953453, -0.010108205489814281, 0.007506772875785828, -0.009772536344826221, -0.005393585655838251, 0.03835777938365936, 0.016249416396021843, 0.034482330083847046, 0.015341585502028465, -0.003509263740852475, 0.010115833953022957, -0.0024011756759136915, ...
d36d548254b36c5cd0874c275e1d48cffe7b9e5d
subsection
39
51
Scattering matrix
Suppose OR|Vga|OR=IRRRaaVga+ILRLabVgb IRRRaa+ILRLab, and OL|Vgb|OL=IRLRbaVga+ILLLbbVgb IRLRba+ILLLbb, where {{\mathsf {O}}}_{{{\mathcal {R}}},{{\mathcal {L}}}} \equiv \sqrt{|{{\mathtt {V}_g}}_{{\mathsf {a}},{\mathsf {b}},{\mathsf {b}}}|}{\widetilde{{\mathsf {O}}}}_{{{\mathcal {R}}},{{\mathcal {L}}}} and {{\mathsf...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ 0.01107238233089447, 0.04554099217057228, -0.04181712865829468, -0.011545496061444283, 0.00956147164106369, -0.018939802423119545, -0.021595342084765434, 0.037818558514118195, 0.044838953763246536, 0.009431746788322926, -0.006387032568454742, 0.0035998597741127014, 0.007829265668988228, 0....
d74147a72a003cf3e18f533345b29c2730526521
subsection
40
51
Scattering matrix
With {{\mathsf {O}}}=[{{\mathsf {O}}}^1_{{{\mathcal {R}}}}~ \cdots ~ {{\mathsf {O}}}^{N^{{{\mathcal {R}}}}}_{{{\mathcal {R}}}}~ {{\mathsf {O}}}^1_{{{\mathcal {L}}}}~ \cdots ~ {{\mathsf {O}}}^{N^{{{\mathcal {L}}}}}_{{{\mathcal {L}}}}]^T, {{\mathsf {I}}}=[{{\mathsf {I}}}^1_{{{\mathcal {R}}}}~ \cdots ~ {{\mathsf {I}}}^{N^...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.03083123080432415, 0.042349085211753845, -0.0022825943306088448, 0.01294423546642065, -0.01035843975841999, -0.00781841017305851, 0.009397347457706928, 0.02663598768413067, 0.044973019510507584, 0.023920519277453423, -0.007780271116644144, 0.001083135837689042, 0.0396336168050766, 0.012...
0d28a593e18dd890b8aebf5701f278f4932b90dc
subsection
41
51
Scattering matrix
As a necessary consequence of the unitarity of \mathbf {S} it follows that \sum \nolimits _{{{\mathsf {a}}}=1}^{N^{{{\mathcal {R}}}}}|{{\tau }}^{{{\mathcal {R}}}\tilde{{{\mathcal {R}}}}}_{{\mathsf {a}}\tilde{{\mathsf {a}}}}|^2+\sum \nolimits _{{{\mathsf {b}}}=1}^{N^{{{\mathcal {L}}}}}|{{\tau }}^{{{\mathcal {L}}}\tilde{...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.04357065260410309, 0.019451184198260307, -0.02158699929714203, 0.0007632682682015002, -0.016018621623516083, -0.020549602806568146, -0.017086530104279518, 0.02895556576550007, -0.008680567145347595, 0.013386990875005722, -0.0231125820428133, 0.015416016802191734, 0.0013053269358351827, ...
b25fcab524e8390d3f36426a7764bd2e8f367e9d
subsection
42
51
Conductance
Finally, the conductance for the transmission from right to left can be expressed at a given frequency {} as GLR=a=1NRTLR which equals that for transmission from left to right given by {{G}}_{{{{\mathcal {L}}}}\rightarrow {{{\mathcal {R}}}}}=\sum _{\tilde{{\mathsf {b}}}=1}^{N^{{\mathcal {L}}}}{{T}}_{{{\mathcal {L}}}\r...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.05723712593317032, 0.007909768261015415, -0.037466518580913544, 0.005690151359885931, 0.007284308783710003, -0.03774110972881317, -0.020533360540866852, 0.01662805676460266, -0.02613198198378086, 0.003113946644589305, -0.016567036509513855, 0.03575794771313667, 0.015552571974694729, 0.0...
7af0afc834a9bdb00ddf8edcf716c04a10984773
subsection
43
51
Concluding remarks
A closed form expression has been provided for the conductance in partly unzipped tubes of square and triangular lattice, and in fact the same form of expression holds. An exact solution of the wave propagation problem has been harnessed for this purpose. A provision of the reflection and transmission coefficients usin...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.02996526099741459, -0.004653464537113905, -0.058404795825481415, 0.019956497475504875, -0.012930529192090034, -0.010634311474859715, 0.03362700343132019, 0.005645186640322208, -0.01368576381355524, 0.033749062567949295, -0.007331114262342453, -0.0003065755881834775, 0.009863818995654583, ...
a36c0c48570d71b5e4760e089802c10a120e3363
subsection
44
51
Body
The discrete Fourier transform {\mathtt {u}}_{{\mathtt {y}}}^F: {\mathbb {C}}\rightarrow {\mathbb {C}} of \lbrace {\mathtt {u}}_{{\mathtt {x}}, {\mathtt {y}}}\rbrace _{{\mathtt {x}}\in {\mathbb {Z}}} (along the {\mathtt {x}} axis) is defined by {\mathtt {u}}_{{\mathtt {y}}}^F={\mathtt {u}}_{{\mathtt {y}};+}+{\mathtt {u...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.029180336743593216, 0.02823411300778389, -0.03090490773320198, -0.013002953492105007, 0.020862720906734467, -0.03017234615981579, 0.0300349909812212, -0.009103593416512012, 0.009279103018343449, 0.05515572056174278, 0.004830322694033384, 0.025715935975313187, -0.013521851040422916, 0.02...
cebf43ae9ef67ecab8cab12da7b9b296e0ba1836
subsection
45
51
Body
Using the definition of Chebyshev polynomial of the second kind, for 0<n\in {\mathbb {Z}}, it follows that {\lambda }^{-n}-{\lambda }^{n}=({\lambda }^{-1}-{\lambda }){\mathtt {U}}_{n-1}({\frac{1}{2}}({\lambda }+{\lambda }^{-1})).Due to their frequent appearance in the rest of the paper, it is also useful to define zP...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.06054455786943436, 0.01956101879477501, -0.05111498758196831, 0.031981196254491806, 0.011840367689728737, 0.00008993996743811294, 0.023116180673241615, -0.027541060000658035, -0.03295772150158882, 0.0014438076177611947, -0.011626752093434334, 0.04003753140568733, -0.02656453475356102, 0...
4e7aef24a1ab27bee8cd8d99a892fd134884a259
subsection
46
51
Body
Since J({{z}}) is bounded on the complex plane and tends to zero as {{z}} tends to 0, it follows that J\equiv 0.Recall that the incident wave is {{\mathrm {A}}}{{a}}_{({{{\kappa }}^{i}}){{\mathtt {y}}}}e^{i{}_x {{\mathtt {x}}}} on the physical sub-lattice, while the incident wave is -{{\mathrm {A}}}{{a}}_{({{{\kappa }}...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.046283408999443054, 0.039235636591911316, -0.02231793850660324, -0.004687072243541479, 0.04070011153817177, -0.012577676214277744, 0.016612600535154343, 0.010297066532075405, -0.035238850861787796, 0.026391001418232918, -0.004668003413826227, 0.024056999012827873, -0.04527658224105835, ...
f549b2c087896bd66f8d6e5c4b788cf58d8bfefa
subsection
47
51
Body
Similarly, for incidence from the unzipped portion, -qF(z)=x=0+ z-x(uix, 0-uix-1, -1)+x=-1+ z-x(uix, 0-uix+1, -1)=Aa(i)0(1+z)(1zP-1)D+(zzP-1).The simplification of (1+{{z}}^{-1})({\mathtt {u}}_+({{z}})+{\mathtt {u}}_-({{z}})), stated in (REF ), is detailed as follows (1+z-1)uF(z)= -12Aa(i)0zP-1(L+(z)z(1L+(z)-l+0)+1-(...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.031061377376317978, 0.0340515673160553, -0.04891099035739899, -0.027186334133148193, 0.0010002267081290483, 0.0034821999724954367, 0.08628838509321213, 0.027918625622987747, -0.0354551263153553, 0.009382489137351513, -0.004592079669237137, 0.0018211944261565804, -0.05028403550386429, 0....
decefc1f64596d683fc20af7697df36c8486b0b7
subsection
48
51
Wiener–Hopf factorization:
Following , assuming that |{{z}}_{{F}}|<1, {{z}}_{{F}}\in {\mathbb {C}}, let {{F}}({{z}}; {{z}}_{{F}}){:=}{{z}}_{{F}}^{-1}(1-{{z}}_{{F}}{{z}})(1-{{z}}_{{F}}{{z}}^{-1}), and {{F}}_\pm ({{z}}; {{z}}_{{F}})={{z}}_{{F}}^{-{\frac{1}{2}}}(1-{{z}}_{{F}}{{z}}^{\mp 1}). The Wiener–Hopf kernel (REF ) can be expressed as \operato...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.054667118936777115, 0.037574104964733124, -0.05808572098612785, 0.009065401740372181, -0.0034949106629937887, 0.018832838162779808, 0.05292729660868645, 0.03632265329360962, -0.043159857392311096, 0.010812857188284397, -0.003105739364400506, 0.019824843853712082, -0.025288503617048264, ...
7f6a6c7a9a22ba7b97af0e941b90a8bc9ddaf665
subsection
49
51
Wiener–Hopf factorization:
For example, in case of the periodic boundary, i.e. {\mathfrak {T}\hspace{-1.69997pt}}{\mathbin {{{\circledcirc }\\{\circ }}}}, the expressions of {{N}} and {{D}} (REF ) can be found to be N(z)=j=1N(6-(z2+z-2)-322-2(z+z-1)jN+1) -2j=1N-1(6-(z2+z-2)-322-2(z+z-1)jN)D(z)=j=1N(6-(z2+z-2)-322-2(z+z-1)2j2N+1), which indica...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ -0.035554442554712296, 0.009865213185548782, -0.04953207075595856, 0.02934386022388935, -0.009666841477155685, 0.011482711881399155, 0.024491365998983383, -0.0007882443023845553, -0.021546296775341034, 0.004871569108217955, 0.000786336837336421, 0.010170402005314827, -0.030732467770576477, ...
419e2d43484a20933f79f3232de61c2ad08b7681
subsection
50
51
Chebyshev polynomials
The Chebyshev polynomials, following Appendix A of , are: first kind {\mathtt {T}}_n= {\frac{1}{2}}(({\vartheta }+\sqrt{{\vartheta }^2-1})^n+({\vartheta }-\sqrt{{\vartheta }^2-1})^n), second kind {\mathtt {U}}_n={\frac{1}{2}}(({\vartheta }+\sqrt{{\vartheta }^2-1})^n-({\vartheta }-\sqrt{{\vartheta }^2-1})^n)/\sqrt{{\va...
{ "cite_spans": [] }
1808.01873
Kinematically restricted phonon transmission in partly-unzipped tubes of square and triangular lattices
[ "Basant Lal Sharma" ]
[ "cond-mat.mes-hall", "math-ph", "math.MP" ]
2,018
en
Physics
[ 0.012876282446086407, 0.007792134303599596, -0.04705030471086502, 0.019802624359726906, -0.017453160136938095, -0.001442670007236302, 0.05306126922369003, -0.00877234898507595, 0.014226461760699749, -0.005046007689088583, -0.028147798031568527, 0.007963767275214195, -0.001682956120930612, ...
2f8774125d402aa817046e3b0ba6971e7a77a8e5
abstract
0
50
Abstract
We classify those rational maps $f: \mathbb{P}^1 \to \mathbb{P}^1$ for which there exists a contravariant tensor $q$ which is parallel, i.e. such that $f^*q // q$, by proving that such maps preserve a parabolic orbifold.
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.047053948044776917, 0.022153804078698158, 0.029187485575675964, -0.025632500648498535, 0.00460011838003993, -0.04503996670246124, 0.026425888761878014, 0.018278414383530617, 0.03664837405085564, 0.045436661690473557, -0.011687199585139751, -0.0031811764929443598, -0.01412076223641634, -...
c79aaa199b86966159f992285710faf6d9ed5972
subsection
1
50
Introduction
A holomorphic dynamical system on the Riemann sphere \mathbb {P}^1 is the data of a rational map f:\mathbb {P}^1\rightarrow \mathbb {P}^1. From the viewpoint of Dynamics, the principal object of interest is the study of the space of orbits \mathbb {P}^1/f under the equivalence relation generated by f, namely z \sim w i...
{ "cite_spans": [ { "arxiv_id": "", "doi": "10.1007/bf02685881", "end": 1123, "openalex_id": "https://openalex.org/W2057221822", "raw": "P. Deligne, Théorie de Hodge. III, Inst. Hautes Études Sci. Publ. Math., (1974), pp. 5–77.", "source_ref_id": "22a4d6ba3e06effe44d3e4553335a2...
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.04963807389140129, 0.03636667877435684, -0.016993489116430283, -0.007245877757668495, 0.032095424830913544, -0.02451394870877266, 0.03194287791848183, 0.004461935255676508, 0.04234643280506134, 0.028754692524671555, -0.029029274359345436, 0.01792401261627674, -0.008939124643802643, -0.0...
98c79570d54a5539ce1f5673066a16843bb25bd7
subsection
2
50
Introduction
This led us to ask for which maps f:\mathbb {P}^1\rightarrow \mathbb {P}^1 does there exist a non-zero meromorphic global section q of \Omega _{\mathbb {P}^1}^{\otimes k} and a constant \lambda \in * such that:f^*q=\lambda qwherein we employ the standard convention, , of identifying A_f of a differential with its image...
{ "cite_spans": [ { "arxiv_id": "", "doi": "10.1007/bf02685881", "end": 321, "openalex_id": "https://openalex.org/W2057221822", "raw": "P. Deligne, Théorie de Hodge. III, Inst. Hautes Études Sci. Publ. Math., (1974), pp. 5–77.", "source_ref_id": "22a4d6ba3e06effe44d3e4553335a22...
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.0721910148859024, 0.024378960952162743, 0.021922757849097252, -0.03441735729575157, 0.024058587849140167, -0.042075831443071365, 0.018886830657720566, -0.005465433932840824, 0.03255613520741463, 0.017086630687117577, -0.009824813343584538, 0.003834957256913185, -0.0072084227576851845, 0...
f2d6d64e0031e4179a55bdc7388fa058e75dbbae
subsection
3
50
A simple case
The space Rat(d) of all rational maps f:\mathbb {P}^1\rightarrow \mathbb {P}^1 with deg(f)=d, is never a group unless d=1, i.e. the group of automorphisms of the complex projective line PGL_2(.The subgroup generated by f \in PGL_2( is clearly isomorphic to \mathbb {Z}, and it acts on \mathbb {P}^1 through[row sep=0.6pc...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.060525063425302505, 0.025211146101355553, -0.012323244474828243, -0.04798053205013275, 0.00534515967592597, -0.02611154317855835, 0.038793422281742096, -0.026813548058271408, 0.03299424797296524, -0.00019839279411826283, -0.017061779275536537, -0.005131505895406008, -0.01120919268578291, ...
0f5d5e16ba9a8d807fe9dfcc7955ac127a769e88
subsection
4
50
A simple case
It follows that \alpha is a primitive n-th root of unity, and as f^*q=\lambda q we see easily that \lambda =\alpha ^j for some j<n.Note that the action of f: \mathbb {G}_m \rightarrow \mathbb {G}_m is a free action, so the quotient map p: \mathbb {G}_m \rightarrow \mathbb {G}_m/f is canonically a \mu _n-torsor.DefineQ(...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.030020682141184807, 0.031180018559098244, -0.0013738505076617002, -0.027213871479034424, 0.032705459743738174, -0.018610382452607155, 0.01932734064757824, 0.014476437121629715, 0.02634437009692192, 0.031103746965527534, -0.03334614634513855, 0.012020477093756199, -0.02761048637330532, 0...
bb1e1290ec3c1ada02142012e410b13da7a1e815
subsection
5
50
A simple case
Since f is an automorphism, for any x \in \mathbb {P}^1 we have ord_x(q)=ord_{f(x)}(q), hence for any k \in \mathbb {Z} the sets S_k=\lbrace x\in \mathbb {P}^1: ord_x(q)=k\rbrace are completely invariant for the dynamics, i.e. f^{-1}(S_k)=S_k.From REF we deduce easily that in Case 1) the only finite set which is comple...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.04454679414629936, 0.04231945425271988, -0.0044279820285737514, -0.03627817705273628, 0.003962681628763676, -0.032403215765953064, 0.04707925021648407, 0.015728680416941643, 0.035240788012742996, 0.030480992048978806, -0.01368440967053175, -0.003348637605085969, -0.018673039972782135, 0...
8d4e043fa160e678976504a077a080e2e6393f92
subsection
6
50
A simple case
Q \in H^0(\mathbb {G}_m/f,\Omega ^{\otimes k}\otimes L_{\lambda }^{-1}) where L_{\lambda } denotes the sheaf on \mathbb {G}_m/f given by the action on the trivial sheaf A_f(f^*1)=\lambda .Thus “multiplication by Q” yields an f-invariant isomorphism of sheaves on \mathbb {G}_m\mathcal {O}\mathop {\longrightarrow }\limit...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.06351986527442932, 0.04625173658132553, 0.005144590511918068, -0.026481864973902702, 0.013912131078541279, -0.006193339359015226, -0.006292493548244238, -0.0006344931316561997, -0.011501915752887726, 0.001129788695834577, -0.01474350318312645, 0.010517998598515987, -0.01171547919511795, ...
e762d5acd2076a5cc72f36ab8dc5c07c9c7066ee
subsection
7
50
Dynamical systems on the Riemann sphere with a parallel tensor
In the holomorphic category, a non-unit endomorphism of \mathbb {P}^1 is a rational map f: \mathbb {P}^1\rightarrow \mathbb {P}^1 of degree d>1. We denote by \Omega _{\mathbb {P}^1} the sheaf of holomorphic differential forms on \mathbb {P}^1, given by the canonical action dz \rightarrow f^{\prime }(z)\,dz, and by \Ome...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.041957564651966095, 0.02897360548377037, -0.01806463859975338, -0.019620882347226143, 0.012892414815723896, -0.01833926886320114, 0.0210703257471323, -0.010931852273643017, 0.037777066230773926, 0.006144875660538673, -0.0123736672103405, 0.00927643571048975, -0.014326600357890129, -0.00...
7ebfb96bdf53daaa8bdfeb35a1a86c2a12c3e524
subsection
8
50
Dynamical systems on the Riemann sphere with a parallel tensor
Within this notation we have f^*q=q(s^n)\,(ns^{n-1}ds)^k and it follows easily thatord_y(f^*q)=deg_y(f)(ord_x(q) +k) -k.Now Assumption REF clearly implies that ord_y(f^*q)=ord_y(q), so we obtain\forall x \in \mathbb {P}^1, \qquad ord_x(q)=deg_x(f)(ord_{f(x)}(q) +k) -k
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.025737281888723373, 0.008390933275222778, -0.04546360298991203, -0.036340370774269104, 0.008688430301845074, -0.04015443101525307, 0.04744691401720047, 0.008596892468631268, 0.030451461672782898, 0.024440500885248184, -0.023845506832003593, -0.018948253244161606, -0.03658447042107582, 0...
81d8fc0198818ab49c6fb92bb2997615c27e1adf
subsection
9
50
Considerations on zeroes and poles
In this section we are going to show that (REF ) constrains the number of zeroes and poles of q.Lemma 3.2 Let f: \mathbb {P}^1\rightarrow \mathbb {P}^1 be a rational map of degree d>1 which satisfies Assumption REF .Then q has no zeroes, that is the set Z:=\lbrace x \in \mathbb {P}^1: ord_x(q) >0 \rbrace is the empty ...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.06956574320793152, -0.010900158435106277, -0.01598791591823101, -0.03618638962507248, 0.008253303356468678, -0.015232761390507221, 0.029168792068958282, 0.024149686098098755, 0.00343633396551013, -0.005861981306225061, -0.04414983466267586, 0.016170984134078026, 0.019664525985717773, -0...
ea9772994b665536645622fbc67301b55e34ed89
subsection
10
50
Considerations on zeroes and poles
Given a zero x \in Z of q with ord_x(q)=e>0, we see from (REF ) that for any y \in f^{-1}(x), setting n:=deg_y(f), we have ord_y(q)=ne + k(n-1)>0, i.e. y \in Z.Observe now that, from the definition of f^*\mathcal {Z}, we haveord_y(f^*q)=ord_y(f^*\mathcal {Z}) + k(n-1) \ge ord_y(f^*\mathcal {Z})Thus summing (REF ) over ...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.041768670082092285, 0.0006321363616734743, -0.05366770923137665, -0.06626848131418228, 0.02361501194536686, 0.023584501817822456, 0.06144784763455391, 0.03703956678509712, 0.012890622951090336, 0.032249439507722855, -0.03905325010418892, 0.020167341455817223, -0.023553991690278053, 0.03...
002ada786f2f19c517a552fbf6e83fd00af4ea91
subsection
11
50
Considerations on zeroes and poles
Moreover we have -ord_y(q) -k= deg_y(f)(-ord_x(q)-k) = ord_y(f^* \mathcal {P}_k), so that,deg(\mathcal {P}_k)= \sum \limits _{x \in P_k} (-ord_x(q) -k) \ge & \sum \limits _{y \in f^{-1}(P_k) } (-ord_y(q) -k) = \\ \sum \limits _{y \in f^{-1}(P_k) } ord_y(f^* \mathcal {P}_k)= deg(f^* \mathcal {P}_k)= & d \cdot deg(\mathc...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.014942570589482784, 0.00021297835337463766, -0.04015196114778519, -0.08738238364458084, 0.009862554259598255, 0.008199726231396198, 0.029091866686940193, 0.04695582762360573, 0.014088273979723454, 0.01993868313729763, -0.03789417818188667, 0.029244419187307358, -0.009854926727712154, 0....
60aa0c5d9c9342735086c6e6e5dec958c5061e92
subsection
12
50
Considerations on zeroes and poles
From deg(f^*\mathcal {P}_m)= d\, deg(\mathcal {P}_m) and d>1, we deduce that deg(\mathcal {P}_m)=0, which implies (REF ).In this section we are going to show that (REF ) constrains the number of zeroes and poles of q.Lemma 3.2 Let f: \mathbb {P}^1\rightarrow \mathbb {P}^1 be a rational map of degree d>1 which satisfie...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.06740158796310425, -0.023688239976763725, -0.026374535635113716, -0.046735431998968124, 0.006601265165954828, -0.0041286526247859, 0.028816621750593185, 0.026206642389297485, 0.006879815831780434, -0.00043499667663127184, -0.039439696818590164, 0.029274513944983482, 0.017430393025279045, ...
4f15f174bf78319349c1f5247411bc8ac51a8ffb
subsection
13
50
Considerations on zeroes and poles
Given a zero x \in Z of q with ord_x(q)=e>0, we see from (REF ) that for any y \in f^{-1}(x), setting n:=deg_y(f), we have ord_y(q)=ne + k(n-1)>0, i.e. y \in Z.Observe now that, from the definition of f^*\mathcal {Z}, we haveord_y(f^*q)=ord_y(f^*\mathcal {Z}) + k(n-1) \ge ord_y(f^*\mathcal {Z})Thus summing (REF ) over ...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.041768670082092285, 0.0006321363616734743, -0.05366770923137665, -0.06626848131418228, 0.02361501194536686, 0.023584501817822456, 0.06144784763455391, 0.03703956678509712, 0.012890622951090336, 0.032249439507722855, -0.03905325010418892, 0.020167341455817223, -0.023553991690278053, 0.03...
bfe2acbab219e47e2eaba3bf7b5700d20deea4a4
subsection
14
50
Considerations on zeroes and poles
Moreover we have -ord_y(q) -k= deg_y(f)(-ord_x(q)-k) = ord_y(f^* \mathcal {P}_k), so that,deg(\mathcal {P}_k)= \sum \limits _{x \in P_k} (-ord_x(q) -k) \ge & \sum \limits _{y \in f^{-1}(P_k) } (-ord_y(q) -k) = \\ \sum \limits _{y \in f^{-1}(P_k) } ord_y(f^* \mathcal {P}_k)= deg(f^* \mathcal {P}_k)= & d \cdot deg(\mathc...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.01928962767124176, 0.0012427999172359705, -0.039769597351551056, -0.08796314150094986, 0.007565532345324755, 0.011773692443966866, 0.03114725463092327, 0.04691164195537567, 0.015344715677201748, 0.019167540594935417, -0.037205785512924194, 0.03378736972808838, -0.004143301863223314, 0.0...
f4f4edb3ae78cc3621aad19eb934df836cc964da
subsection
15
50
Main Lemma: the dynamical system preserves a parabolic orbifold
In this section we discuss the main consequence of Assumption REF , i.e. the existence of an orbifold or eventually an orbifold with boundary that is preserved by f. We refer to and to for a formal definition of an orbifold. Observe that under our hypothesis, given any ramification point x\in Ram_f, its image f(x) is ...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 226, "openalex_id": "", "raw": "W. P. Thurston, Three-dimensional geometry and topology. Vol. 1, vol. 35 of Princeton Mathematical Series, Princeton University Press, Princeton, NJ, 1997. Edited by Silvio Levy.", "source_ref...
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.04777955636382103, 0.010991433635354042, -0.009687107056379318, -0.03368367254734039, -0.012860206887125969, -0.04652862250804901, 0.03810770437121391, 0.029412193223834038, 0.05867183208465576, 0.009206565096974373, -0.016018051654100418, 0.00601058267056942, -0.0035049021244049072, 0....
579174d5bb42a34ab86db52518d2393c22e5acaa
subsection
16
50
Main Lemma: the dynamical system preserves a parabolic orbifold
Then f preserves one of the following parabolic orbifolds (resp. orbifold with boundary):(\infty ,\infty ) (2,2,\infty ) (2,2,2,2) (3,3,3) (2,4,4) (2,3,6)It is a fact that, for q a meromorphic global section of the sheaf \Omega _{\mathbb {P}^1}^{\otimes k}, we have\sum \limits _{x \in \mathbb {P}^1} ord_x(q)= deg(...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.024299971759319305, 0.02457454800605774, 0.0027019036933779716, -0.059552472084760666, 0.005827111657708883, -0.014926253817975521, 0.04994231462478638, 0.02335420995950699, 0.029608439654111862, 0.034321993589401245, 0.0024044462479650974, 0.004995756782591343, -0.023796582594513893, 0...
68724600fec0334b79b405e6a2adae34b2c66ebf
subsection
17
50
Main Lemma: the dynamical system preserves a parabolic orbifold
\end{array}\right.}It follows from the discussion above that \nu _f satisfies condition (REF ), so f preserves an orbifold with boundary of type (ii).Our aim is now to show that any solution of (REF ) with n_k=0 corresponds to one of the orbifold (iii)-(vi) listed above. Note that we must have n_i\le 4, \;\forall i and...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.028636060655117035, 0.033075641840696335, -0.007918015122413635, -0.041954804211854935, 0.005026948172599077, -0.026652742177248, 0.04500606283545494, 0.023494688794016838, 0.052023954689502716, 0.02058073878288269, -0.004531118553131819, 0.018002424389123917, -0.014478221535682678, 0.0...
03bb3130f1b4590b9facc25b48f3dc77520405e0
subsection
18
50
Main Lemma: the dynamical system preserves a parabolic orbifold
In fact, note that if n_i=2 then there is only another nonzero n_j solving (REF ), hence n_j \alpha _j=2(1-\alpha _i) and consequently, if \alpha _i > \frac{3}{4}, we should have n_j \alpha _j < \frac{1}{2} which is impossible. Note that \alpha _i\ne \frac{2}{3}, otherwise we would have n_i=3.We claim that there are no...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.04710285738110542, 0.024787764996290207, -0.0025852385442703962, -0.051101867109537125, -0.011333075352013111, 0.016224995255470276, 0.012370986863970757, 0.01238625030964613, 0.034831080585718155, 0.0005890718894079328, -0.015843410044908524, 0.005735223181545734, 0.018972408026456833, ...
fb4c2a20015fe3840df0d89db235754082d9b82e
subsection
19
50
Main Lemma: the dynamical system preserves a parabolic orbifold
Thus we have \nu _f(y)deg_y(f)=4 in each case, so we conclude that f preserves an orbifold of type (v).Finally we suppose that n_i\le 1,\;\forall i. It is clear that in this case we must have \#\lbrace i:n_i\ne 0\rbrace =3, so we can rewrite equation (REF ) in the form \alpha + \beta + \gamma =2, with \alpha ,\beta ,\g...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.01352658960968256, 0.01094028726220131, -0.015189756639301777, -0.06719808280467987, 0.013671544380486012, -0.041563935577869415, 0.024505022913217545, 0.0251916516572237, 0.0502612367272377, 0.008788850158452988, -0.019790170714259148, 0.0150142852216959, -0.021239720284938812, 0.01910...
0825e2869ede135b10d700e0dd4447198f2a187b
subsection
20
50
Main Lemma: the dynamical system preserves a parabolic orbifold
It follows that \nu _f(y)deg_y(f)=6 in each case, so \nu _f satisfies condition (REF ), i.e. f preserves an orbifold of type (vi).\textbf {Remark} 3.6 We have shown that every solution of (REF ) with \alpha _i \ne 1 is such that \alpha _i=\left(1-\frac{1}{n}\right) for some n=2,3,4 \mbox{ or } 6, i.e. q may only have...
{ "cite_spans": [ { "arxiv_id": "", "doi": "", "end": 1116, "openalex_id": "", "raw": "W. P. Thurston, Three-dimensional geometry and topology. Vol. 1, vol. 35 of Princeton Mathematical Series, Princeton University Press, Princeton, NJ, 1997. Edited by Silvio Levy.", "source_re...
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.005244331434369087, 0.01638519950211048, -0.005846953019499779, -0.059712912887334824, 0.008238368667662144, -0.029490306973457336, 0.045249998569488525, 0.01650724932551384, 0.06297774612903595, 0.012197362259030342, 0.0036500548012554646, 0.014073879458010197, -0.013127991929650307, 0...
eadc19c2dbdd8d0deab26c1ebbc835899c85e477
subsection
21
50
Main Lemma: the dynamical system preserves a parabolic orbifold
Also, we denote by \mathcal {O}=(\mathbb {P}^1, \nu _f) the orbifold preserved by f and we shall refer to it, for brevity's sake, through the string (\nu _f(x)\mathop {)}_{x \in P_f}.By definition if \nu _f takes the value \infty we will say that \mathcal {O} is an orbifold with boundary, which we will denote by (\mat...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.03894321620464325, 0.04660367965698242, -0.001059608068317175, -0.04870954155921936, -0.012940379790961742, -0.03451785072684288, 0.04773290827870369, 0.0186628345400095, 0.03955361247062683, 0.03955361247062683, -0.025834979489445686, 0.012383393943309784, -0.0008526458987034857, 0.011...
fa5e7ac0491c92e69656b8fdc9165aec286167f7
subsection
22
50
Main Lemma: the dynamical system preserves a parabolic orbifold
We proved in REF that the set of poles of q of order k is a complete invariant set for the dynamics, hence in the first case if we define\nu _f(x)= {\left\lbrace \begin{array}{ll} \infty , & \mbox{if } ord_x(q)=k;\\ 1, & \mbox{otherwise}. \end{array}\right.}it is clear that \nu _f satisfies condition (REF ), i.e f pres...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.0362800695002079, 0.026637930423021317, -0.007277372758835554, -0.050041474401950836, 0.008841169066727161, -0.052329953759908676, 0.0494617223739624, 0.016766944900155067, 0.05095686390995979, 0.032374393194913864, 0.011007598601281643, 0.009893870912492275, -0.018338369205594063, 0.03...
c20cc1d5d903fba1404adfaa6cf4003fe6b12e28
subsection
23
50
Main Lemma: the dynamical system preserves a parabolic orbifold
Therefore n_i=3 for some i if and only if \alpha _i=\frac{2}{3} (note that it makes sense only if k\equiv 0\;(mod\, 3)). In this case let P=\lbrace p_1,p_2,p_3\rbrace be the set of poles of q, each of order \frac{2}{3} k and let us define\nu _f(x)= {\left\lbrace \begin{array}{ll} 3, & \mbox{if } x \in P; \\ 1, & \mbox{...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.029885048046708107, 0.0164840929210186, 0.004361416213214397, -0.07185843586921692, 0.002571823773905635, -0.023398254066705704, 0.010623081587255001, 0.0014099241234362125, 0.02385614439845085, 0.015934621915221214, -0.0034799750428646803, 0.016560407355427742, -0.0005289600230753422, ...
03f96dc6e411b319f7426d7cade56ebf2d799364
subsection
24
50
Main Lemma: the dynamical system preserves a parabolic orbifold
By the Riemann-Hurwitz formula, the ramification of a rational map of degree d has order 2d-2, hence we obtain 2d-2=(e_1-1)+\dots +(e_r-1)=d-(r+s), which is absurd since d>1.Therefore we conclude that n_i=2 for some i \ne k, \frac{k}{2} if and only if \alpha _i=\frac{3}{4} (note that it makes sense only if k \equiv 0 ...
{ "cite_spans": [] }
1806.10056
Dynamical systems with a parallel tensor
[ "Jacopo Garofali" ]
[ "math.DS" ]
2,018
en
Mathematics
[ -0.04507887735962868, 0.03839487209916115, 0.008324484340846539, -0.041446931660175323, -0.018739627674221992, -0.0117656784132123, 0.03659415990114212, 0.011086596176028252, 0.04901603236794472, 0.022081630304455757, -0.025393111631274223, 0.004631496034562588, 0.012582103721797466, 0.024...