Holographic Schwinger-Keldysh effective field theories

Abstract We construct a holographic dual of the Schwinger-Keldysh effective action for the dissipative low-energy dynamics of relativistic charged matter at strong coupling in a fixed thermal background. To do so, we use a mixed signature bulk spacetime whereby an eternal asymptotically anti-de Sitt...

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Main Authors: Jan de Boer, Michal P. Heller, Natalia Pinzani-Fokeeva
Format: Article
Language:English
Published: SpringerOpen 2019-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP05(2019)188
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author Jan de Boer
Michal P. Heller
Natalia Pinzani-Fokeeva
author_facet Jan de Boer
Michal P. Heller
Natalia Pinzani-Fokeeva
author_sort Jan de Boer
collection DOAJ
description Abstract We construct a holographic dual of the Schwinger-Keldysh effective action for the dissipative low-energy dynamics of relativistic charged matter at strong coupling in a fixed thermal background. To do so, we use a mixed signature bulk spacetime whereby an eternal asymptotically anti-de Sitter black hole is glued to its Euclidean counterpart along an initial time slice in a way to match the desired double-time contour of the dual field theory. Our results are consistent with existing literature and can be regarded as a fully-ab initio derivation of a Schwinger-Keldysh effective action. In addition, we provide a simple infrared effective action for the near horizon region that drives all the dissipation and can be viewed as an alternative to the membrane paradigm approximation.
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spelling doaj.art-9cf58e5b39ba477d9775dd38138286ac2022-12-21T17:59:00ZengSpringerOpenJournal of High Energy Physics1029-84792019-05-012019514110.1007/JHEP05(2019)188Holographic Schwinger-Keldysh effective field theoriesJan de Boer0Michal P. Heller1Natalia Pinzani-Fokeeva2Institute for Theoretical Physics, University of AmsterdamMax Planck Institute for Gravitational PhysicsInstitute for Theoretical Physics, KU LeuvenAbstract We construct a holographic dual of the Schwinger-Keldysh effective action for the dissipative low-energy dynamics of relativistic charged matter at strong coupling in a fixed thermal background. To do so, we use a mixed signature bulk spacetime whereby an eternal asymptotically anti-de Sitter black hole is glued to its Euclidean counterpart along an initial time slice in a way to match the desired double-time contour of the dual field theory. Our results are consistent with existing literature and can be regarded as a fully-ab initio derivation of a Schwinger-Keldysh effective action. In addition, we provide a simple infrared effective action for the near horizon region that drives all the dissipation and can be viewed as an alternative to the membrane paradigm approximation.http://link.springer.com/article/10.1007/JHEP05(2019)188AdS-CFT CorrespondenceEffective Field Theories
spellingShingle Jan de Boer
Michal P. Heller
Natalia Pinzani-Fokeeva
Holographic Schwinger-Keldysh effective field theories
Journal of High Energy Physics
AdS-CFT Correspondence
Effective Field Theories
title Holographic Schwinger-Keldysh effective field theories
title_full Holographic Schwinger-Keldysh effective field theories
title_fullStr Holographic Schwinger-Keldysh effective field theories
title_full_unstemmed Holographic Schwinger-Keldysh effective field theories
title_short Holographic Schwinger-Keldysh effective field theories
title_sort holographic schwinger keldysh effective field theories
topic AdS-CFT Correspondence
Effective Field Theories
url http://link.springer.com/article/10.1007/JHEP05(2019)188
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AT michalpheller holographicschwingerkeldysheffectivefieldtheories
AT nataliapinzanifokeeva holographicschwingerkeldysheffectivefieldtheories