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

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dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, M.
dc.contributor.authorTahamtan, T.
dc.date.accessioned2026-02-06T18:51:17Z
dc.date.issued2013
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWe find Einstein-Yang-Mills (EYM) black hole solutions endowed with massless scalar hair in the presence of a potential V(phi) as function of the scalar field phi. Choosing V(phi) = 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 asymptotically go in general to any known limits. A particular case is given, however, which admits an asymptotically anti-de Sitter limit in 6-dimensional spacetime. The role of the potential V(phi) in making double bounces (i.e. both a minimum and maximum radii) on a domain wall universe is highlighted.
dc.identifier.doi10.1140/epjc/s10052-012-2264-y
dc.identifier.issn1434-6044
dc.identifier.issue1
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.orcid0000-0002-3204-7722
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.scopus2-s2.0-84872084869
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjc/s10052-012-2264-y
dc.identifier.urihttps://hdl.handle.net/11129/15264
dc.identifier.volume73
dc.identifier.wosWOS:000318288100005
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer
dc.relation.ispartofEuropean Physical Journal C
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectGeneral-Relativity
dc.subjectThin Shells
dc.titleDouble-bounce domain wall in Einstein-Yang-Mills-Scalar black holes
dc.typeArticle

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