Black hole solutions in f(R) gravity coupled with non-linear Yang-Mills field

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dc.contributor.author Mazharimousavi, S. Habib
dc.contributor.author Halilsoy, Mustafa
dc.date.accessioned 2016-01-07T14:21:59Z
dc.date.available 2016-01-07T14:21:59Z
dc.date.issued 2011
dc.identifier.citation S. Habib Mazharimousavi and M. Halilsoy (2011) arXiv:1105.3659 "Black hole solutions in f(R) gravity coupled with non-linear Yang-Mills eld", Phys. Rev. D 84 (2011) 064032. en_US
dc.identifier.issn 1550-7998
dc.identifier.other DOI: 10.1103/PhysRevD.84.064032
dc.identifier.uri http://hdl.handle.net/11129/1942
dc.description The file in this item is the publisher version (published version) of the article. en_US
dc.description.abstract It is shown that in the static, spherically symmetric spacetime the problem of metric f(R) gravity coupled with non-linear Yang-Mills (YM) field constructed from the Wu-Yang ansatz as source, can be solved in all dimensions. By non-linearity it is meant that the YM Lagrangian depends arbitrarily on its invariant. A particular form is considered to be in the power-law form with limit of the standard YM theory. The formalism admits black hole solutions with single or double horizons in which f(R) can be obtained, in general numerically. In 6-dimensional case we obtain an exact solution given by f(R)=\surdR gravity that couples with the YM field in a consistent manner. 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 84, 064032 (2011)
dc.subject general relativity en_US
dc.subject black holes en_US
dc.title Black hole solutions in f(R) gravity coupled with non-linear Yang-Mills field en_US
dc.type Article en_US
dc.description.version Publisher Version (Published Version).


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