The holographic shape of entanglement and Einstein’s equations

Abstract We study shape-deformations of the entanglement entropy and the modular Hamiltonian for an arbitrary subregion and state (with a smooth dual geometry) in a holographic conformal field theory. More precisely, we study a double-deformation comprising of a shape deformation together with a sta...

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Main Authors: Aitor Lewkowycz, Onkar Parrikar
Format: Article
Language:English
Published: SpringerOpen 2018-05-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP05(2018)147
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spelling doaj-a832179c98294008a40278ec126bc4432020-11-25T00:27:30ZengSpringerOpenJournal of High Energy Physics1029-84792018-05-012018513310.1007/JHEP05(2018)147The holographic shape of entanglement and Einstein’s equationsAitor Lewkowycz0Onkar Parrikar1Stanford Institute for Theoretical Physics, Deptartment of Physics, Stanford UniversityDavid Rittenhouse Laboratory, University of PennsylvaniaAbstract We study shape-deformations of the entanglement entropy and the modular Hamiltonian for an arbitrary subregion and state (with a smooth dual geometry) in a holographic conformal field theory. More precisely, we study a double-deformation comprising of a shape deformation together with a state deformation, where the latter corresponds to a small change in the bulk geometry. Using a purely gravitational identity from the Hollands-Iyer-Wald formalism together with the assumption of equality between bulk and boundary modular flows for the original, undeformed state and subregion, we rewrite a purely CFT expression for this double deformation of the entropy in terms of bulk gravitational variables and show that it precisely agrees with the Ryu-Takayanagi formula including quantum corrections. As a corollary, this gives a novel, CFT derivation of the JLMS formula for arbitrary subregions in the vacuum, without using the replica trick. Finally, we use our results to give an argument that if a general, asymptotically AdS spacetime satisfies the Ryu-Takayanagi formula for arbitrary subregions, then it must necessarily satisfy the non-linear Einstein equation.http://link.springer.com/article/10.1007/JHEP05(2018)147AdS-CFT CorrespondenceConformal Field Theory
collection DOAJ
language English
format Article
sources DOAJ
author Aitor Lewkowycz
Onkar Parrikar
spellingShingle Aitor Lewkowycz
Onkar Parrikar
The holographic shape of entanglement and Einstein’s equations
Journal of High Energy Physics
AdS-CFT Correspondence
Conformal Field Theory
author_facet Aitor Lewkowycz
Onkar Parrikar
author_sort Aitor Lewkowycz
title The holographic shape of entanglement and Einstein’s equations
title_short The holographic shape of entanglement and Einstein’s equations
title_full The holographic shape of entanglement and Einstein’s equations
title_fullStr The holographic shape of entanglement and Einstein’s equations
title_full_unstemmed The holographic shape of entanglement and Einstein’s equations
title_sort holographic shape of entanglement and einstein’s equations
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2018-05-01
description Abstract We study shape-deformations of the entanglement entropy and the modular Hamiltonian for an arbitrary subregion and state (with a smooth dual geometry) in a holographic conformal field theory. More precisely, we study a double-deformation comprising of a shape deformation together with a state deformation, where the latter corresponds to a small change in the bulk geometry. Using a purely gravitational identity from the Hollands-Iyer-Wald formalism together with the assumption of equality between bulk and boundary modular flows for the original, undeformed state and subregion, we rewrite a purely CFT expression for this double deformation of the entropy in terms of bulk gravitational variables and show that it precisely agrees with the Ryu-Takayanagi formula including quantum corrections. As a corollary, this gives a novel, CFT derivation of the JLMS formula for arbitrary subregions in the vacuum, without using the replica trick. Finally, we use our results to give an argument that if a general, asymptotically AdS spacetime satisfies the Ryu-Takayanagi formula for arbitrary subregions, then it must necessarily satisfy the non-linear Einstein equation.
topic AdS-CFT Correspondence
Conformal Field Theory
url http://link.springer.com/article/10.1007/JHEP05(2018)147
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