Gravitational entropy of a Kerr black hole

The gravitational entropy of a Kerr black hole is calculated using a classical estimator based on the Bel-Robinson tensor, which has been recently proposed by Clifton, Ellis, and Tavakol. We prove that, in the frame we consider, Clifton et al.’s estimator does not reproduce the Bekenstein-Hawking en...

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Autores principales: Pérez, Daniela, Romero, Gustavo Esteban
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2014
Materias:
Ciencias Astronómicas
black hole
gravitational entropy
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/165273
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SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-165273
record_format dspace
spelling I19-R120-10915-1652732024-04-24T20:07:58Z http://sedici.unlp.edu.ar/handle/10915/165273 Gravitational entropy of a Kerr black hole Pérez, Daniela Romero, Gustavo Esteban 2014-04 2015 2024-04-24T17:35:34Z en Ciencias Astronómicas black hole gravitational entropy The gravitational entropy of a Kerr black hole is calculated using a classical estimator based on the Bel-Robinson tensor, which has been recently proposed by Clifton, Ellis, and Tavakol. We prove that, in the frame we consider, Clifton et al.’s estimator does not reproduce the Bekenstein-Hawking entropy of a Kerr black hole. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 133-138
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
black hole
gravitational entropy
spellingShingle Ciencias Astronómicas
black hole
gravitational entropy
Pérez, Daniela
Romero, Gustavo Esteban
Gravitational entropy of a Kerr black hole
topic_facet Ciencias Astronómicas
black hole
gravitational entropy
description The gravitational entropy of a Kerr black hole is calculated using a classical estimator based on the Bel-Robinson tensor, which has been recently proposed by Clifton, Ellis, and Tavakol. We prove that, in the frame we consider, Clifton et al.’s estimator does not reproduce the Bekenstein-Hawking entropy of a Kerr black hole.
format Objeto de conferencia
Objeto de conferencia
author Pérez, Daniela
Romero, Gustavo Esteban
author_facet Pérez, Daniela
Romero, Gustavo Esteban
author_sort Pérez, Daniela
title Gravitational entropy of a Kerr black hole
title_short Gravitational entropy of a Kerr black hole
title_full Gravitational entropy of a Kerr black hole
title_fullStr Gravitational entropy of a Kerr black hole
title_full_unstemmed Gravitational entropy of a Kerr black hole
title_sort gravitational entropy of a kerr black hole
publishDate 2014
url http://sedici.unlp.edu.ar/handle/10915/165273
work_keys_str_mv AT perezdaniela gravitationalentropyofakerrblackhole
AT romerogustavoesteban gravitationalentropyofakerrblackhole
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