Thermodynamics of charged anti-de Sitter black holes in canonical ensemble

As in the grand canonical treatment of Reissner-Nordstrom black holes in anti-de Sitter spacetime, the canonical ensemble formulation also shows that non-extremal black holes tend to have lower action than extremal ones. However, $9 some small non-extremal black holes have higher action, leading to...

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Detalles Bibliográficos
Autor principal: Mitra, P.
Lenguaje:eng
Publicado: 1999
Materias:
General Relativity and Cosmology
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(99)00689-9
http://cds.cern.ch/record/409854
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author Mitra, P.
author_facet Mitra, P.
author_sort Mitra, P.
collection CERN
description As in the grand canonical treatment of Reissner-Nordstrom black holes in anti-de Sitter spacetime, the canonical ensemble formulation also shows that non-extremal black holes tend to have lower action than extremal ones. However, $9 some small non-extremal black holes have higher action, leading to the possibility of transitions between non- extremal and extremal black holes. (9 refs).
id cern-409854
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
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spelling cern-4098542023-03-14T18:44:43Zdoi:10.1016/S0370-2693(99)00689-9http://cds.cern.ch/record/409854engMitra, P.Thermodynamics of charged anti-de Sitter black holes in canonical ensembleGeneral Relativity and CosmologyAs in the grand canonical treatment of Reissner-Nordstrom black holes in anti-de Sitter spacetime, the canonical ensemble formulation also shows that non-extremal black holes tend to have lower action than extremal ones. However, $9 some small non-extremal black holes have higher action, leading to the possibility of transitions between non- extremal and extremal black holes. (9 refs).As in the grand canonical treatment of Reissner–Nordström black holes in anti-de Sitter spacetime, the canonical ensemble formulation also shows that non-extremal black holes tend to have lower action than extremal ones. However, some small non-extremal black holes have higher action, leading to the possibility of transitions between non-extremal and extremal black holes.As in the grand canonical treatment of Reissner - Nordstr\"{o}m black holes in anti-de Sitter spacetime, the canonical ensemble formulation also shows that non-extremal black holes tend to have lower action than extremal ones. However, some small non-extremal black holes have higher action, leading to the possibility of transitions between non-extremal and extremal black holes.gr-qc/9903078oai:cds.cern.ch:4098541999
spellingShingle General Relativity and Cosmology
Mitra, P.
Thermodynamics of charged anti-de Sitter black holes in canonical ensemble
title Thermodynamics of charged anti-de Sitter black holes in canonical ensemble
title_full Thermodynamics of charged anti-de Sitter black holes in canonical ensemble
title_fullStr Thermodynamics of charged anti-de Sitter black holes in canonical ensemble
title_full_unstemmed Thermodynamics of charged anti-de Sitter black holes in canonical ensemble
title_short Thermodynamics of charged anti-de Sitter black holes in canonical ensemble
title_sort thermodynamics of charged anti-de sitter black holes in canonical ensemble
topic General Relativity and Cosmology
url https://dx.doi.org/10.1016/S0370-2693(99)00689-9
http://cds.cern.ch/record/409854
work_keys_str_mv AT mitrap thermodynamicsofchargedantidesitterblackholesincanonicalensemble

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