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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Online Access: | http://link.springer.com/article/10.1007/JHEP07(2018)050 |
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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 |
work_keys_str_mv |
AT xidong desitterholographyandentanglemententropy AT evasilverstein desitterholographyandentanglemententropy AT gonzalotorroba desitterholographyandentanglemententropy |
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1725204655951052800 |