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A thermal product formula

We show that holographic thermal two-sided two-point correlators take the form of a product over quasi-normal modes (QNMs). Due to this fact, the two-point function admits a natural dispersive representation with a positive discontinuity at the location of QNMs. We explore the general constraints on...

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Detalles Bibliográficos
Autores principales: Dodelson, Matthew, Iossa, Cristoforo, Karlsson, Robin, Zhiboedov, Alexander
Lenguaje:eng
Publicado: 2023
Materias:
Acceso en línea:http://cds.cern.ch/record/2857001
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author Dodelson, Matthew
Iossa, Cristoforo
Karlsson, Robin
Zhiboedov, Alexander
author_facet Dodelson, Matthew
Iossa, Cristoforo
Karlsson, Robin
Zhiboedov, Alexander
author_sort Dodelson, Matthew
collection CERN
description We show that holographic thermal two-sided two-point correlators take the form of a product over quasi-normal modes (QNMs). Due to this fact, the two-point function admits a natural dispersive representation with a positive discontinuity at the location of QNMs. We explore the general constraints on the structure of QNMs that follow from the operator product expansion, the presence of the singularity inside the black hole, and the hydrodynamic expansion of the correlator. We illustrate these constraints through concrete examples. We suggest that the product formula for thermal correlators may hold for more general large N chaotic systems, and we check this hypothesis in several models.
id cern-2857001
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2023
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spelling cern-28570012023-09-20T06:40:02Zhttp://cds.cern.ch/record/2857001engDodelson, MatthewIossa, CristoforoKarlsson, RobinZhiboedov, AlexanderA thermal product formulagr-qcGeneral Relativity and Cosmologycond-mat.str-elcond-mat.stat-mechhep-thParticle Physics - TheoryWe show that holographic thermal two-sided two-point correlators take the form of a product over quasi-normal modes (QNMs). Due to this fact, the two-point function admits a natural dispersive representation with a positive discontinuity at the location of QNMs. We explore the general constraints on the structure of QNMs that follow from the operator product expansion, the presence of the singularity inside the black hole, and the hydrodynamic expansion of the correlator. We illustrate these constraints through concrete examples. We suggest that the product formula for thermal correlators may hold for more general large N chaotic systems, and we check this hypothesis in several models.arXiv:2304.12339CERN-TH-2023-062oai:cds.cern.ch:28570012023-04-24
spellingShingle gr-qc
General Relativity and Cosmology
cond-mat.str-el
cond-mat.stat-mech
hep-th
Particle Physics - Theory
Dodelson, Matthew
Iossa, Cristoforo
Karlsson, Robin
Zhiboedov, Alexander
A thermal product formula
title A thermal product formula
title_full A thermal product formula
title_fullStr A thermal product formula
title_full_unstemmed A thermal product formula
title_short A thermal product formula
title_sort thermal product formula
topic gr-qc
General Relativity and Cosmology
cond-mat.str-el
cond-mat.stat-mech
hep-th
Particle Physics - Theory
url http://cds.cern.ch/record/2857001
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AT karlssonrobin athermalproductformula
AT zhiboedovalexander athermalproductformula
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AT iossacristoforo thermalproductformula
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AT zhiboedovalexander thermalproductformula