Lovelock black holes with a power-Yang-Mills source

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dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.date.accessioned	2016-01-20T11:50:34Z
dc.date.available	2016-01-20T11:50:34Z
dc.date.issued	2009
dc.identifier.citation	S. Habib Mazharimousavi and Mustafa Halilsoy, (2009): arXiv:0908.0308 "Lovelockblack holes with a power-Yang-Mills source". Physics Letters B 681 (2009) 190 -199.	en_US
dc.identifier.issn	1873-2445 (online)
dc.identifier.issn	0370-2693 (print)
dc.identifier.other	DOI: 10.1016/j.physletb.2009.10.006
dc.identifier.uri	http://hdl.handle.net/11129/2020
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	We consider the standard Yang-Mills (YM) invariant raised to the power q, i.e., (F(a)μνF(a)μν)q as the source of our geometry and investigate the possible black hole solutions. How does this parameter q modify the black holes in Einstein-Yang-Mills (EYM) and its extensions such as Gauss-Bonnet (GB) and the third order Lovelock theories? The advantage of such a power q (or a set of superposed members of the YM hierarchies) if any, may be tested even in a free YM theory in flat spacetime. Our choice of the YM field is purely magnetic in any higher dimensions so that duality makes no sense. In analogy with the Einstein-power-Maxwell theory, the conformal invariance provides further reduction, albeit in a spacetime for dimensions of multiples of 4.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Physics Letters B, Elsevier	en_US
dc.relation.ispartofseries	Elsevier;Phys.Lett.B681:190-199,2009
dc.subject	gravity	en_US
dc.subject	general relativity	en_US
dc.subject	power-Yang-Mills source	en_US
dc.subject	Lovelock black holes	en_US
dc.title	Lovelock black holes with a power-Yang-Mills source	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).