Constant curvature f(R) gravity minimally coupled with Yang-Mills field

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dc.contributor.author Mazharimousavi, S. Habib
dc.contributor.author Halilsoy, Mustafa
dc.contributor.author Tahamtan, Tayebeh
dc.date.accessioned 2016-01-07T12:37:17Z
dc.date.available 2016-01-07T12:37:17Z
dc.date.issued 2011
dc.identifier.citation “Constant curvature f(R) gravity minimally coupled with Yang – Mills field”. S. H. Mazharimousavi, M. Halilsoy, T. Tahamtan, Eur. Phys. J.C (2011), 72:1958. en_US
dc.identifier.issn 1434-6052 (online)
dc.identifier.issn 1434-6044 (print)
dc.identifier.other DOI: 10.1140/epjc/s10052-012-1958-5
dc.identifier.uri http://hdl.handle.net/11129/1936
dc.description The file in this item is the publisher version (published version) of the article. en_US
dc.description.abstract We consider the particular class of f(R) gravities minimally coupled with Yang - Mills (YM) field in which the Ricci scalar =R_{0}= constant in all dimensions d\geq4. Even in this restricted class the spacetime has unlimited scopes determined by an equation of state of the form P_{eff}={\omega}{\rho}. Depending on the distance from the origin (or horizon of a black hole) the state function {\omega}(r) takes different values. It is observed that {\omega}\rightarrow(1/3) (the ultra relativistic case in 4 - dimensions) and {\omega}\rightarrow-1 (the cosmological constant) are the limiting values of our state function {\omega}(r) in a spacetime centered by a black hole. This suggests that having a constant {\omega} throughout spacetime around a charged black hole in f(R) gravity with constant scalar curvature is a myth. en_US
dc.language.iso en_US en_US
dc.publisher European Physical Journal C, Springer en_US
dc.relation.ispartofseries Springer;Eur. Phys. J. C (2012) 72:1958
dc.subject general relativity en_US
dc.subject black holes en_US
dc.subject f(r) Gravity en_US
dc.subject Yang-Mills field en_US
dc.title Constant curvature f(R) gravity minimally coupled with Yang-Mills field en_US
dc.type Article en_US
dc.description.version Publisher Version (Published Version).


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