{"title":"Integrable Multi-Hamiltonian Systems from Reduction of an Extended Quasi-Poisson Double of ({text {U}}(n))","authors":"M. Fairon, L. Fehér","doi":"10.1007/s00023-023-01344-8","DOIUrl":"10.1007/s00023-023-01344-8","url":null,"abstract":"<div><p>We construct a master dynamical system on a <span>({text {U}}(n))</span> quasi-Poisson manifold, <span>({mathcal {M}}_d)</span>, built from the double <span>({text {U}}(n) times {text {U}}(n))</span> and <span>(dge 2)</span> open balls in <span>(mathbb {C}^n)</span>, whose quasi-Poisson structures are obtained from <span>(T^* mathbb {R}^n)</span> by exponentiation. A pencil of quasi-Poisson bivectors <span>(P_{underline{z}})</span> is defined on <span>({mathcal {M}}_d)</span> that depends on <span>(d(d-1)/2)</span> arbitrary real parameters and gives rise to pairwise compatible Poisson brackets on the <span>({text {U}}(n))</span>-invariant functions. The master system on <span>({mathcal {M}}_d)</span> is a quasi-Poisson analogue of the degenerate integrable system of free motion on the extended cotangent bundle <span>(T^*!{text {U}}(n) times mathbb {C}^{ntimes d})</span>. Its commuting Hamiltonians are pullbacks of the class functions on one of the <span>({text {U}}(n))</span> factors. We prove that the master system descends to a degenerate integrable system on a dense open subset of the smooth component of the quotient space <span>({mathcal {M}}_d/{text {U}}(n))</span> associated with the principal orbit type. Any reduced Hamiltonian arising from a class function generates the same flow via any of the compatible Poisson structures stemming from the bivectors <span>(P_{underline{z}})</span>. The restrictions of the reduced system on minimal symplectic leaves parameterized by generic elements of the center of <span>({text {U}}(n))</span> provide a new real form of the complex, trigonometric spin Ruijsenaars–Schneider model of Krichever and Zabrodin. This generalizes the derivation of the compactified trigonometric RS model found previously in the <span>(d=1)</span> case.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 10","pages":"3461 - 3529"},"PeriodicalIF":1.5,"publicationDate":"2023-07-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-023-01344-8.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"6713726","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Morawetz Estimates Without Relative Degeneration and Exponential Decay on Schwarzschild–de Sitter Spacetimes","authors":"Georgios Mavrogiannis","doi":"10.1007/s00023-023-01293-2","DOIUrl":"10.1007/s00023-023-01293-2","url":null,"abstract":"<div><p>We use a novel physical space method to prove <i>relatively</i> non-degenerate integrated energy estimates for the wave equation on subextremal Schwarzschild–de?Sitter spacetimes with parameters <span>((M,Lambda ))</span>. These are integrated decay statements whose bulk energy density, though degenerate at highest order, is everywhere comparable to the energy density of the boundary fluxes. As a corollary, we prove that solutions of the wave equation decay exponentially on the exterior region. The main ingredients are a previous Morawetz estimate of Dafermos–Rodnianski and an additional argument based on commutation with a vector field which can be expressed in the form </p><div><div><span>$$begin{aligned} rsqrt{1-frac{2M}{r}-frac{Lambda }{3}r^2}frac{partial }{partial r}, end{aligned}$$</span></div></div><p>where <span>(partial _r)</span> here denotes the coordinate vector field corresponding to a well-chosen system of hyperboloidal coordinates. Our argument gives exponential decay also for small first-order perturbations of the wave operator. In the limit <span>(Lambda =0)</span>, our commutation corresponds to the one introduced by Holzegel–Kauffman (A note on the wave equation on black hole spacetimes with small non-decaying first-order terms, 2020. arXiv:2005.13644).</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 9","pages":"3113 - 3152"},"PeriodicalIF":1.5,"publicationDate":"2023-06-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-023-01293-2.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4800279","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Transition Amplitudes in 3D Quantum Gravity: Boundaries and Holography in the Coloured Boulatov Model","authors":"Christophe Goeller, Daniele Oriti, Gabriel Schmid","doi":"10.1007/s00023-023-01330-0","DOIUrl":"10.1007/s00023-023-01330-0","url":null,"abstract":"<div><p>We consider transition amplitudes in the coloured simplicial Boulatov model for three-dimensional Riemannian quantum gravity. First, we discuss aspects of the topology of coloured graphs with non-empty boundaries. Using a modification of the standard rooting procedure of coloured tensor models, we then write transition amplitudes systematically as topological expansions. We analyse the transition amplitudes for the simplest boundary topology, the 2-sphere, and prove that they factorize into a sum entirely given by the combinatorics of the boundary spin network state and that the leading order is given by graphs representing the closed 3-ball in the large <i>N</i> limit. This is the first step towards a more detailed study of the holographic nature of coloured Boulatov-type GFT models for topological field theories and quantum gravity.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 10","pages":"3601 - 3684"},"PeriodicalIF":1.5,"publicationDate":"2023-06-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-023-01330-0.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"6713794","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"({hat{Z}})-Invariant for SO(3) and OSp(1|2) Groups","authors":"Sachin Chauhan, Pichai Ramadevi","doi":"10.1007/s00023-023-01332-y","DOIUrl":"10.1007/s00023-023-01332-y","url":null,"abstract":"<div><p>Three-manifold invariants <span>({hat{Z}})</span> (“<i>Z</i>-hat”), also known as homological blocks, are <i>q</i>-series with integer coefficients. Explicit <i>q</i>-series form for <span>({hat{Z}})</span> is known for <i>SU</i>(2) group, supergroup <i>SU</i>(2|1) and orthosymplectic supergroup <i>OSp</i>(2|2). We focus on <span>({hat{Z}})</span> for <i>SO</i>(3) group and orthosymplectic supergroup <i>OSp</i>(1|2) in this paper. Particularly, the change of variable relating <i>SU</i>(2) link invariants to the <i>SO</i>(3) and <i>OSp</i>(1|2) link invariants plays a crucial role in explicitly writing the <i>q</i>-series.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 10","pages":"3347 - 3371"},"PeriodicalIF":1.5,"publicationDate":"2023-06-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"6713782","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Price’s Law and Precise Late-Time Asymptotics for Subextremal Reissner–Nordström Black Holes","authors":"Yannis Angelopoulos, Stefanos Aretakis, Dejan Gajic","doi":"10.1007/s00023-023-01328-8","DOIUrl":"10.1007/s00023-023-01328-8","url":null,"abstract":"<div><p>In this paper, we prove precise late-time asymptotics for solutions to the wave equation supported on angular frequencies greater or equal to <span>(ell )</span> on the domain of outer communications of subextremal Reissner–Nordstr?m spacetimes up to and including the event horizon. Our asymptotics yield, in particular, sharp upper and lower decay rates which are consistent with Price’s law on such backgrounds. We present a theory for inverting the time operator and derive an explicit representation of the leading-order asymptotic coefficient in terms of the Newman–Penrose charges at null infinity associated with the time integrals. Our method is based on purely physical space techniques. For each angular frequency <span>(ell )</span>, we establish a sharp hierarchy of <i>r</i>-weighted radially commuted estimates with length <span>(2ell +5)</span>. We complement this hierarchy with a novel hierarchy of weighted elliptic estimates of length <span>(ell +1)</span>.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 9","pages":"3215 - 3287"},"PeriodicalIF":1.5,"publicationDate":"2023-06-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4089257","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"The Quantization of Proca Fields on Globally Hyperbolic Spacetimes: Hadamard States and Møller Operators","authors":"Valter Moretti, Simone Murro, Daniele Volpe","doi":"10.1007/s00023-023-01326-w","DOIUrl":"10.1007/s00023-023-01326-w","url":null,"abstract":"<div><p>This paper deals with several issues concerning the algebraic quantization of the real Proca field in a globally hyperbolic spacetime and the definition and existence of Hadamard states for that field. In particular, extending previous work, we construct the so-called M?ller <span>(*)</span>-isomorphism between the algebras of Proca observables on paracausally related spacetimes, proving that the pullback of these isomorphisms preserves the Hadamard property of corresponding quasifree states defined on the two spacetimes. Then, we pull back a natural Hadamard state constructed on ultrastatic spacetimes of bounded geometry, along this <span>(*)</span>-isomorphism, to obtain an Hadamard state on a general globally hyperbolic spacetime. We conclude the paper, by comparing the definition of an Hadamard state, here given in terms of wavefront set, with the one proposed by Fewster and Pfenning, which makes use of a supplementary Klein–Gordon Hadamard form. We establish an (almost) complete equivalence of the two definitions.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 9","pages":"3055 - 3111"},"PeriodicalIF":1.5,"publicationDate":"2023-05-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-023-01326-w.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"5130187","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Quand Galilée et Carroll engendrent Lorentz","authors":"Jean-Marc Lévy-Leblond","doi":"10.1007/s00023-023-01321-1","DOIUrl":"10.1007/s00023-023-01321-1","url":null,"abstract":"<div><h2>Résumé</h2><div><p>Le présent article montre l’existence d’une inédite relation suggestive entre le groupe de Lorentz et ses cousins dégénérés, les groupes de Galilée et de Carroll.</p></div></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 9","pages":"3209 - 3213"},"PeriodicalIF":1.5,"publicationDate":"2023-05-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4584868","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Hanno Gottschalk, Nicolai R. Rothe, Daniel Siemssen
{"title":"Cosmological de Sitter Solutions of the Semiclassical Einstein Equation","authors":"Hanno Gottschalk, Nicolai R. Rothe, Daniel Siemssen","doi":"10.1007/s00023-023-01315-z","DOIUrl":"10.1007/s00023-023-01315-z","url":null,"abstract":"<div><p>Exponentially expanding space–times play a central role in contemporary cosmology, most importantly in the theory of inflation and in the dark energy driven expansion in the late universe. In this work, we give a complete list of de Sitter solutions of the semiclassical Einstein equation (SCE), where classical gravity is coupled to the expected value of a renormalized stress–energy tensor of a free quantum field in the Bunch–Davies state. To achieve this, we explicitly determine the stress–energy tensor associated with the Bunch–Davies state using the recently proposed “moment approach” on the cosmological coordinate patch of de Sitter space. From the energy component of the SCE, we thus obtain an analytic consistency equation for the model’s parameters which has to be fulfilled by solutions to the SCE. Using this equation, we then investigate the number of solutions and the structure of the solution set in dependency on the coupling parameter of the quantum field to the scalar curvature and renormalization constants using analytic arguments in combination with numerical evidence. We also identify parameter sets where multiple expansion rates separated by several orders of magnitude are possible. Potentially for such parameter settings, a fast (semi-stable) expansion in the early universe could be compatible with a late-time “Dark Energy-like” behavior of the universe.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 9","pages":"2949 - 3029"},"PeriodicalIF":1.5,"publicationDate":"2023-05-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-023-01315-z.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4394112","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Henning Bostelmann, Daniela Cadamuro, Christoph Minz
{"title":"On the Mass Dependence of the Modular Operator for a Double Cone","authors":"Henning Bostelmann, Daniela Cadamuro, Christoph Minz","doi":"10.1007/s00023-023-01311-3","DOIUrl":"10.1007/s00023-023-01311-3","url":null,"abstract":"<div><p>We present a numerical approximation scheme for the Tomita–Takesaki modular operator of local subalgebras in linear quantum fields, working at one-particle level. This is applied to the local subspaces for double cones in the vacuum sector of a massive scalar free field in <span>((1+1))</span>- and <span>((3+1))</span>-dimensional Minkowski spacetime, using a discretization of time-0 data in position space. In the case of a wedge region, one component of the modular generator is well known to be a mass-independent multiplication operator; our results strongly suggest that for the double cone, the corresponding component is still at least close to a multiplication operator, but that it is dependent on mass and angular momentum.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 9","pages":"3031 - 3054"},"PeriodicalIF":1.5,"publicationDate":"2023-05-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00023-023-01311-3.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4515108","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Anisotropic Spin Generalization of Elliptic Macdonald–Ruijsenaars Operators and R-Matrix Identities","authors":"M. Matushko, Andrei Zotov","doi":"10.1007/s00023-023-01316-y","DOIUrl":"10.1007/s00023-023-01316-y","url":null,"abstract":"<div><p>We propose commuting set of matrix-valued difference operators in terms of the elliptic Baxter–Belavin <i>R</i>-matrix in the fundamental representation of <span>(textrm{GL}_M)</span>. In the scalar case <span>(M=1)</span>, these operators are the elliptic Macdonald–Ruijsenaars operators, while in the general case they can be viewed as anisotropic versions of the quantum spin Ruijsenaars Hamiltonians. We show that commutativity of the operators for any <i>M</i> is equivalent to a set of <i>R</i>-matrix identities. The proof of identities is based on the properties of elliptic <i>R</i>-matrix including the quantum and the associative Yang–Baxter equations. As an application of our results, we introduce elliptic version of q-deformed Haldane–Shastry model.</p></div>","PeriodicalId":463,"journal":{"name":"Annales Henri Poincaré","volume":"24 10","pages":"3373 - 3419"},"PeriodicalIF":1.5,"publicationDate":"2023-05-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"6713781","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}