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

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dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, M.
dc.date.accessioned2026-02-06T18:49:02Z
dc.date.issued2012
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractconsider 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.
dc.identifier.doi10.1103/PhysRevD.86.088501
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.issue8
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.scopus2-s2.0-84867073869
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.86.088501
dc.identifier.urihttps://hdl.handle.net/11129/14703
dc.identifier.volume86
dc.identifier.wosWOS:000309386800015
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Physical Soc
dc.relation.ispartofPhysical Review D
dc.relation.publicationcategoryDiğer
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.titleComment on Static and spherically symmetric black holes in f(R) theories''
dc.typeEditorial

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