De Sitter holography and entanglement entropy

Abstract We propose a new example of entanglement knitting spacetime together, satisfying a series of checks of the corresponding von Neumann and Renyi entropies. The conjectured dual of de Sitter in d + 1 dimensions involves two coupled CFT sectors constrained by residual d-dimensional gravity. In...

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Main Authors: Xi Dong, Eva Silverstein, Gonzalo Torroba
Format: Article
Language:English
Published: SpringerOpen 2018-07-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP07(2018)050
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spelling doaj-9ffe9903d8394201bd882366fc4898e62020-11-25T01:02:29ZengSpringerOpenJournal of High Energy Physics1029-84792018-07-012018712410.1007/JHEP07(2018)050De Sitter holography and entanglement entropyXi Dong0Eva Silverstein1Gonzalo Torroba2Department of Physics, University of CaliforniaStanford Institute for Theoretical Physics, Stanford UniversityCentro Atómico Bariloche and CONICETAbstract We propose a new example of entanglement knitting spacetime together, satisfying a series of checks of the corresponding von Neumann and Renyi entropies. The conjectured dual of de Sitter in d + 1 dimensions involves two coupled CFT sectors constrained by residual d-dimensional gravity. In the d = 2 case, the gravitational constraints and the CFT spectrum are relatively tractable. We identify a finite portion of each CFT Hilbert space relevant for de Sitter. Its maximum energy level coincides with the transition to the universal Cardy behavior for theories with a large central charge and a sparse light spectrum, derived by Hartman, Keller, and Stoica. Significant interactions between the two CFTs, derived previously for other reasons, suggest a maximally mixed state upon tracing out one of the two sectors; we derive this by determining the holographic Renyi entropies. The resulting entanglement entropy matches the Gibbons-Hawking formula for de Sitter entropy, including the numerical coefficient. Finally, we interpret the Gibbons-Hawking horizon entropy in terms of the Ryu-Takayanagi entropy, and explore the time evolution of the entanglement entropy.http://link.springer.com/article/10.1007/JHEP07(2018)050Gauge-gravity correspondenceAdS-CFT CorrespondenceConformal Field TheoryBlack Holes
collection DOAJ
language English
format Article
sources DOAJ
author Xi Dong
Eva Silverstein
Gonzalo Torroba
spellingShingle Xi Dong
Eva Silverstein
Gonzalo Torroba
De Sitter holography and entanglement entropy
Journal of High Energy Physics
Gauge-gravity correspondence
AdS-CFT Correspondence
Conformal Field Theory
Black Holes
author_facet Xi Dong
Eva Silverstein
Gonzalo Torroba
author_sort Xi Dong
title De Sitter holography and entanglement entropy
title_short De Sitter holography and entanglement entropy
title_full De Sitter holography and entanglement entropy
title_fullStr De Sitter holography and entanglement entropy
title_full_unstemmed De Sitter holography and entanglement entropy
title_sort de sitter holography and entanglement entropy
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-07-01
description Abstract We propose a new example of entanglement knitting spacetime together, satisfying a series of checks of the corresponding von Neumann and Renyi entropies. The conjectured dual of de Sitter in d + 1 dimensions involves two coupled CFT sectors constrained by residual d-dimensional gravity. In the d = 2 case, the gravitational constraints and the CFT spectrum are relatively tractable. We identify a finite portion of each CFT Hilbert space relevant for de Sitter. Its maximum energy level coincides with the transition to the universal Cardy behavior for theories with a large central charge and a sparse light spectrum, derived by Hartman, Keller, and Stoica. Significant interactions between the two CFTs, derived previously for other reasons, suggest a maximally mixed state upon tracing out one of the two sectors; we derive this by determining the holographic Renyi entropies. The resulting entanglement entropy matches the Gibbons-Hawking formula for de Sitter entropy, including the numerical coefficient. Finally, we interpret the Gibbons-Hawking horizon entropy in terms of the Ryu-Takayanagi entropy, and explore the time evolution of the entanglement entropy.
topic Gauge-gravity correspondence
AdS-CFT Correspondence
Conformal Field Theory
Black Holes
url http://link.springer.com/article/10.1007/JHEP07(2018)050
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AT evasilverstein desitterholographyandentanglemententropy
AT gonzalotorroba desitterholographyandentanglemententropy
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