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Ruppeiner theory of black hole thermodynamics

The Ruppeiner metric as determined by the Hessian of the Gibbs surface provides a geometric description of thermodynamic systems in equilibrium. An interesting example is a black hole in equilibrium with its own Hawking radiation. In this article, we present results from the Ruppeiner study of vario...

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Autores principales: Aman, Jan E, Bedford, James, Grumiller, Daniel, Pidokrajt, Narit, Ward, John
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1742-6596/66/1/012007
http://cds.cern.ch/record/1000915
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author Aman, Jan E
Bedford, James
Grumiller, Daniel
Pidokrajt, Narit
Ward, John
author_facet Aman, Jan E
Bedford, James
Grumiller, Daniel
Pidokrajt, Narit
Ward, John
author_sort Aman, Jan E
collection CERN
description The Ruppeiner metric as determined by the Hessian of the Gibbs surface provides a geometric description of thermodynamic systems in equilibrium. An interesting example is a black hole in equilibrium with its own Hawking radiation. In this article, we present results from the Ruppeiner study of various black hole families from different gravity theories e.g. 2D dilaton gravity, BTZ, general relativity and higher-dimensional Einstein-Maxwell gravity.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2006
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spelling cern-10009152023-03-14T18:14:15Zdoi:10.1088/1742-6596/66/1/012007http://cds.cern.ch/record/1000915engAman, Jan EBedford, JamesGrumiller, DanielPidokrajt, NaritWard, JohnRuppeiner theory of black hole thermodynamicsGeneral Relativity and CosmologyThe Ruppeiner metric as determined by the Hessian of the Gibbs surface provides a geometric description of thermodynamic systems in equilibrium. An interesting example is a black hole in equilibrium with its own Hawking radiation. In this article, we present results from the Ruppeiner study of various black hole families from different gravity theories e.g. 2D dilaton gravity, BTZ, general relativity and higher-dimensional Einstein-Maxwell gravity.The Ruppeiner metric as determined by the Hessian of the Gibbs surface provides a geometric description of thermodynamic systems in equilibrium. An interesting example is a black hole in equilibrium with its own Hawking radiation. In this article, we present results from the Ruppeiner study of various black hole families from different gravity theories e.g. 2D dilaton gravity, BTZ, general relativity and higher-dimensional Einstein-Maxwell gravity.gr-qc/0611119MIT-CTP-3787QMUL-PH-06-09USITP-06-04MIT-CTP-3787QMUL-PH-2006-09USITP-2006-04oai:cds.cern.ch:10009152006-11-22
spellingShingle General Relativity and Cosmology
Aman, Jan E
Bedford, James
Grumiller, Daniel
Pidokrajt, Narit
Ward, John
Ruppeiner theory of black hole thermodynamics
title Ruppeiner theory of black hole thermodynamics
title_full Ruppeiner theory of black hole thermodynamics
title_fullStr Ruppeiner theory of black hole thermodynamics
title_full_unstemmed Ruppeiner theory of black hole thermodynamics
title_short Ruppeiner theory of black hole thermodynamics
title_sort ruppeiner theory of black hole thermodynamics
topic General Relativity and Cosmology
url https://dx.doi.org/10.1088/1742-6596/66/1/012007
http://cds.cern.ch/record/1000915
work_keys_str_mv AT amanjane ruppeinertheoryofblackholethermodynamics
AT bedfordjames ruppeinertheoryofblackholethermodynamics
AT grumillerdaniel ruppeinertheoryofblackholethermodynamics
AT pidokrajtnarit ruppeinertheoryofblackholethermodynamics
AT wardjohn ruppeinertheoryofblackholethermodynamics