Thermodynamics of accelerating and supersymmetric AdS4 black holes

We study the thermodynamics of AdS4 black hole solutions of Einstein-Maxwell theory that are accelerating, rotating, and carry electric and magnetic charges. We focus on the class for which the black hole horizon is a spindle and can be uplifted on regular Sasaki-Einstein spaces to give solutions of...

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Main Authors: Martelli, D, Gauntlett, J, Cassani, D, Sparks, JF
Format: Journal article
Language:English
Published: American Physical Society 2021
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author Martelli, D
Gauntlett, J
Cassani, D
Sparks, JF
author_facet Martelli, D
Gauntlett, J
Cassani, D
Sparks, JF
author_sort Martelli, D
collection OXFORD
description We study the thermodynamics of AdS4 black hole solutions of Einstein-Maxwell theory that are accelerating, rotating, and carry electric and magnetic charges. We focus on the class for which the black hole horizon is a spindle and can be uplifted on regular Sasaki-Einstein spaces to give solutions of D = 11 supergravity that are free from conical singularities. We use holography to calculate the Euclidean on-shell action and to define a set of conserved charges which give rise to a first law. We identify a complex locus of supersymmetric and nonextremal solutions, defined through an analytic continuation of the parameters, upon which we obtain a simple expression for the on-shell action. A Legendre transform of this action combined with a reality constraint then leads to the Bekenstein-Hawking entropy for the class of supersymmetric and extremal black holes.
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spelling oxford-uuid:7fd82811-c439-4bdc-a393-d2528d7ebaff2022-03-26T21:19:30ZThermodynamics of accelerating and supersymmetric AdS4 black holesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7fd82811-c439-4bdc-a393-d2528d7ebaffEnglishSymplectic ElementsAmerican Physical Society2021Martelli, DGauntlett, JCassani, DSparks, JFWe study the thermodynamics of AdS4 black hole solutions of Einstein-Maxwell theory that are accelerating, rotating, and carry electric and magnetic charges. We focus on the class for which the black hole horizon is a spindle and can be uplifted on regular Sasaki-Einstein spaces to give solutions of D = 11 supergravity that are free from conical singularities. We use holography to calculate the Euclidean on-shell action and to define a set of conserved charges which give rise to a first law. We identify a complex locus of supersymmetric and nonextremal solutions, defined through an analytic continuation of the parameters, upon which we obtain a simple expression for the on-shell action. A Legendre transform of this action combined with a reality constraint then leads to the Bekenstein-Hawking entropy for the class of supersymmetric and extremal black holes.
spellingShingle Martelli, D
Gauntlett, J
Cassani, D
Sparks, JF
Thermodynamics of accelerating and supersymmetric AdS4 black holes
title Thermodynamics of accelerating and supersymmetric AdS4 black holes
title_full Thermodynamics of accelerating and supersymmetric AdS4 black holes
title_fullStr Thermodynamics of accelerating and supersymmetric AdS4 black holes
title_full_unstemmed Thermodynamics of accelerating and supersymmetric AdS4 black holes
title_short Thermodynamics of accelerating and supersymmetric AdS4 black holes
title_sort thermodynamics of accelerating and supersymmetric ads4 black holes
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AT gauntlettj thermodynamicsofacceleratingandsupersymmetricads4blackholes
AT cassanid thermodynamicsofacceleratingandsupersymmetricads4blackholes
AT sparksjf thermodynamicsofacceleratingandsupersymmetricads4blackholes