A Cardy-like formula for rotating black holes with planar horizon

Abstract We show that the semiclassical entropy of D−dimensional rotating (an)isotropic black holes with planar horizon can be successfully computed according to a Cardy-like formula. This formula does not refer to any central charges but instead involves the vacuum energy which is identified with a...

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Main Authors: Moisés Bravo Gaete, Luis Guajardo, Mokhtar Hassaïne
Format: Article
Language:English
Published: SpringerOpen 2017-04-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP04(2017)092
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author Moisés Bravo Gaete
Luis Guajardo
Mokhtar Hassaïne
author_facet Moisés Bravo Gaete
Luis Guajardo
Mokhtar Hassaïne
author_sort Moisés Bravo Gaete
collection DOAJ
description Abstract We show that the semiclassical entropy of D−dimensional rotating (an)isotropic black holes with planar horizon can be successfully computed according to a Cardy-like formula. This formula does not refer to any central charges but instead involves the vacuum energy which is identified with a gravitational bulk soliton. The soliton is obtained from the non-rotating black hole solution by means of a double analytic continuation. The robustness of the Cardy-like formula is tested with numerous and varied examples, including AdS, Lifshitz and hyperscaling violation planar black holes.
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spelling doaj.art-55a3cb10352f43ddbc85fb4ed61f27452022-12-22T01:23:02ZengSpringerOpenJournal of High Energy Physics1029-84792017-04-012017412610.1007/JHEP04(2017)092A Cardy-like formula for rotating black holes with planar horizonMoisés Bravo Gaete0Luis Guajardo1Mokhtar Hassaïne2Facultad de Ciencias Básicas, Universidad Católica del MauleInstituto de Matemática y Fisica, Universidad de TalcaInstituto de Matemática y Fisica, Universidad de TalcaAbstract We show that the semiclassical entropy of D−dimensional rotating (an)isotropic black holes with planar horizon can be successfully computed according to a Cardy-like formula. This formula does not refer to any central charges but instead involves the vacuum energy which is identified with a gravitational bulk soliton. The soliton is obtained from the non-rotating black hole solution by means of a double analytic continuation. The robustness of the Cardy-like formula is tested with numerous and varied examples, including AdS, Lifshitz and hyperscaling violation planar black holes.http://link.springer.com/article/10.1007/JHEP04(2017)092Black HolesClassical Theories of Gravity
spellingShingle Moisés Bravo Gaete
Luis Guajardo
Mokhtar Hassaïne
A Cardy-like formula for rotating black holes with planar horizon
Journal of High Energy Physics
Black Holes
Classical Theories of Gravity
title A Cardy-like formula for rotating black holes with planar horizon
title_full A Cardy-like formula for rotating black holes with planar horizon
title_fullStr A Cardy-like formula for rotating black holes with planar horizon
title_full_unstemmed A Cardy-like formula for rotating black holes with planar horizon
title_short A Cardy-like formula for rotating black holes with planar horizon
title_sort cardy like formula for rotating black holes with planar horizon
topic Black Holes
Classical Theories of Gravity
url http://link.springer.com/article/10.1007/JHEP04(2017)092
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