The action of geometric entropy in topologically massive gravity

Abstract Due to the presence of a gravitational anomaly in topologically massive gravity (TMG), the geometric entropy is no longer simply the Hubeny-Rangamani-Takayanagi (HRT) area; instead, it is given by the HRT area plus an anomalous contribution. We study the action of this geometric entropy on...

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Main Author: Molly Kaplan
Format: Article
Language:English
Published: SpringerOpen 2023-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2023)106
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author Molly Kaplan
author_facet Molly Kaplan
author_sort Molly Kaplan
collection DOAJ
description Abstract Due to the presence of a gravitational anomaly in topologically massive gravity (TMG), the geometric entropy is no longer simply the Hubeny-Rangamani-Takayanagi (HRT) area; instead, it is given by the HRT area plus an anomalous contribution. We study the action of this geometric entropy on the covariant phase space of classical solutions for TMG with matter fields whose action is algebraic in the metric. The result agrees precisely with the action of HRT area operators in Einstein-Hilbert gravity given in [8], i.e., it is a boundary-condition-preserving kink transformation. Furthermore, we show our result to be consistent with direct computations of semiclassical commutators of geometric entropies in pure TMG spacetimes asymptotic to planar AdS, as computed in [21].
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spelling doaj.art-4989b6ec2a714c36a7d3a842e94777392024-03-31T11:08:22ZengSpringerOpenJournal of High Energy Physics1029-84792023-12-0120231212910.1007/JHEP12(2023)106The action of geometric entropy in topologically massive gravityMolly Kaplan0Department of Physics, University of California at Santa BarbaraAbstract Due to the presence of a gravitational anomaly in topologically massive gravity (TMG), the geometric entropy is no longer simply the Hubeny-Rangamani-Takayanagi (HRT) area; instead, it is given by the HRT area plus an anomalous contribution. We study the action of this geometric entropy on the covariant phase space of classical solutions for TMG with matter fields whose action is algebraic in the metric. The result agrees precisely with the action of HRT area operators in Einstein-Hilbert gravity given in [8], i.e., it is a boundary-condition-preserving kink transformation. Furthermore, we show our result to be consistent with direct computations of semiclassical commutators of geometric entropies in pure TMG spacetimes asymptotic to planar AdS, as computed in [21].https://doi.org/10.1007/JHEP12(2023)106AdS-CFT CorrespondenceChern-Simons TheoriesGauge-Gravity CorrespondenceClassical Theories of Gravity
spellingShingle Molly Kaplan
The action of geometric entropy in topologically massive gravity
Journal of High Energy Physics
AdS-CFT Correspondence
Chern-Simons Theories
Gauge-Gravity Correspondence
Classical Theories of Gravity
title The action of geometric entropy in topologically massive gravity
title_full The action of geometric entropy in topologically massive gravity
title_fullStr The action of geometric entropy in topologically massive gravity
title_full_unstemmed The action of geometric entropy in topologically massive gravity
title_short The action of geometric entropy in topologically massive gravity
title_sort action of geometric entropy in topologically massive gravity
topic AdS-CFT Correspondence
Chern-Simons Theories
Gauge-Gravity Correspondence
Classical Theories of Gravity
url https://doi.org/10.1007/JHEP12(2023)106
work_keys_str_mv AT mollykaplan theactionofgeometricentropyintopologicallymassivegravity
AT mollykaplan actionofgeometricentropyintopologicallymassivegravity