Gravitational entropy of a Schwarzschild-type black hole

dc.authoridDil, Emre/0000-0002-9042-7694
dc.contributor.authorDil, Emre
dc.date.accessioned2025-03-23T19:26:05Z
dc.date.available2025-03-23T19:26:05Z
dc.date.issued2016
dc.departmentSinop Üniversitesi
dc.description.abstractIn this study, Clifton, Ellis and Tavakol's gravitational entropy proposal is used to determine the entropy of free gravitational fields due to a spherical symmetric Schwarzschild-type black hole which is considered in the framework of f(R) gravity. In order to obtain the gravitational entropy, we calculate the Weyl tensor of the black hole to determine the Bel-Robinson tensor, giving the super energy density. By using the super energy density, we obtain the gravitational energy density and the gravitational temperature to calculate the gravitational entropy of the f(R) gravity black hole. This proposal can reproduce the Bekenstein-Hawking value in general relativity limit, but cannot reproduce it in the f(R) gravity case.
dc.identifier.doi10.3938/jkps.69.6
dc.identifier.endpage10
dc.identifier.issn0374-4884
dc.identifier.issn1976-8524
dc.identifier.issue1
dc.identifier.scopus2-s2.0-84978162041
dc.identifier.scopusqualityQ3
dc.identifier.startpage6
dc.identifier.urihttps://doi.org/10.3938/jkps.69.6
dc.identifier.urihttps://hdl.handle.net/11486/4626
dc.identifier.volume69
dc.identifier.wosWOS:000379709900002
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.institutionauthorDil, Emre
dc.language.isoen
dc.publisherKorean Physical Soc
dc.relation.ispartofJournal of the Korean Physical Society
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WOS_20250323
dc.subjectGeneral relativity
dc.subjectGravitation
dc.subjectf(R) gravity
dc.subjectBlack holes
dc.subjectEntropy
dc.titleGravitational entropy of a Schwarzschild-type black hole
dc.typeArticle

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