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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...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2023
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/2857001 |
_version_ | 1780977543868841984 |
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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 |
record_format | invenio |
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 |
work_keys_str_mv | AT dodelsonmatthew athermalproductformula AT iossacristoforo athermalproductformula AT karlssonrobin athermalproductformula AT zhiboedovalexander athermalproductformula AT dodelsonmatthew thermalproductformula AT iossacristoforo thermalproductformula AT karlssonrobin thermalproductformula AT zhiboedovalexander thermalproductformula |