Cargando…
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...
Autores principales: | , , , , |
---|---|
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 |
_version_ | 1780911578014547968 |
---|---|
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. |
id | cern-1000915 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2006 |
record_format | invenio |
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 |