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

dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.date.accessioned	2016-01-07T08:22:51Z
dc.date.available	2016-01-07T08:22:51Z
dc.date.issued	2012
dc.identifier.citation	S. 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.issn	1550-7998
dc.identifier.other	DOI: 10.1103/PhysRevD.86.088501
dc.identifier.uri	http://hdl.handle.net/11129/1927
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	We 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.language.iso	en_US	en_US
dc.publisher	Physical Review D, American Physical Society (APS)	en_US
dc.relation.ispartofseries	;Phys. Rev. D 86, 088501 (2012)
dc.subject	general relativity	en_US
dc.subject	black holes	en_US
dc.title	Comment on "Static and spherically symmetric black holes in f(R) theories"	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).