Double-bounce domain-wall in Einstein-Yang-Mills-Scalar black holes

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dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.contributor.author	Tahamtan, Tayabeh
dc.date.accessioned	2016-01-07T09:17:38Z
dc.date.available	2016-01-07T09:17:38Z
dc.date.issued	2013
dc.identifier.citation	S. Habib Mazharimousavi, M. Halilsoy and T. Tahamtan (2012) arXiv:1207.1644 "Double-bounce domain-wall in Einstein-Yang-Mills-Scalar black holes". Eur. Phys. J. C (2013) 73, 2264.	en_US
dc.identifier.issn	1434-6052 (online)
dc.identifier.issn	1434-6044 (print)
dc.identifier.other	DOI: 10.1140/epjc/s10052-012-2264-y
dc.identifier.uri	http://hdl.handle.net/11129/1929
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	We find Einstein-Yang-Mills (EYM) black hole solutions endowed with massless scalar hair in the presence of a potential V(ϕ) as function of the scalar field ϕ. Choosing V(ϕ)=constant (or zero) sets the scalar field to vanish leaving us with the EYM black holes. Our class of black hole solutions is new so that they do not asymptote in general to any known limits. Particular case is given, however, which admits an asymptotically anti de Sitter limit in 6−dimensional spacetime. The role of the potential V(ϕ) in making double bounces (i.e. both a minimum and maximum radii) on a Domain Wall (DW) universe is highlighted.	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 (2013) 73, 2264
dc.subject	general relativity	en_US
dc.subject	black holes	en_US
dc.title	Double-bounce domain-wall in Einstein-Yang-Mills-Scalar black holes	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).