Comment on "Static and spherically symmetric black holes in f(R) theories"

dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, Mustafa
dc.date.accessioned2016-01-07T08:22:51Z
dc.date.available2016-01-07T08:22:51Z
dc.date.issued2012
dc.descriptionThe file in this item is the publisher version (published version) of the article.en_US
dc.description.abstractWe consider the interesting ‘‘near-horizon test’’ reported in S. E. P. Bergliaffa and Y. E. C. de O. Nunes,Phys. Rev. D 84, 084006 (2011) for any static, spherically symmetric black hole solution admitted in f(R)gravity. Before adopting the necessary conditions for the test, however, revisions are needed as we point out in this Comment.en_US
dc.description.versionPublisher Version (Published Version).
dc.identifier.citationS. HabibMazharimousavi and M. Halilsoy, arXiv:1210.4699. "Comment on "Staticand spherically symmetric black holes in f(R) theories"". Phys. Rev. D 86, 088501 (2012).en_US
dc.identifier.issn1550-7998
dc.identifier.otherDOI: 10.1103/PhysRevD.86.088501
dc.identifier.urihttps://hdl.handle.net/11129/1927
dc.language.isoen
dc.publisherPhysical Review D, American Physical Society (APS)en_US
dc.relation.ispartofseries;Phys. Rev. D 86, 088501 (2012)
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.subjectgeneral relativityen_US
dc.subjectblack holesen_US
dc.titleComment on "Static and spherically symmetric black holes in f(R) theories"en_US
dc.typeArticle

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