N-Dimensional non-abelian dilatonic, stable black holes and their Born-Infeld extension

dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, Mustafa
dc.contributor.authorAmirabi, Zahra
dc.date.accessioned2016-01-20T13:51:33Z
dc.date.available2016-01-20T13:51:33Z
dc.date.issued2009
dc.descriptionThe file in this item is the post-print version of the article (author’s copy; author’s final manuscript, accepted for publication after peer-review process). Due to copyright restrictions, the access to the publisher version (published version) of this article is only available via subscription. You may click URI (with DOI: 10.1007/s10714-009-0835-5) and have access to the Publisher Version of this article through the publisher web site or online databases, if your Library or institution has subscription to the related journal or publication.en_US
dc.description.abstractWe find large classes of non-asymptotically flat Einstein-Yang-Mills-Dilaton (EYMD) and Einstein-Yang-Mills-Born-Infeld-Dilaton (EYMBID) black holes in N-dimensional spherically symmetric spacetime expressed in terms of the quasilocal mass. Extension of the dilatonic YM solution to N-dimensions has been possible by employing the generalized Wu-Yang ansatz. Another metric ansatz, which aided in finding exact solutions is the functional dependence of the radius function on the dilaton field. These classes of black holes are stable against linear radial perturbations. In the limit of vanishing dilaton we obtain Bertotti-Robinson (BR) type metrics with the topology of AdS2×SN−2. Since connection can be established between dilaton and a scalar field of Brans-Dicke (BD) type we obtain black hole solutions also in the Brans-Dicke-Yang-Mills (BDYM) theory as well.en_US
dc.description.versionPost-Print Author Version (Final Author Manuscript, accepted for publication, after peer-review process).
dc.identifier.citationS. Habib Mazharimousavi, Mustafa Halilsoy and Zahra Amirabi, General Relativity and Gravitation 28 (2009) 261: arXiv:0802.3990"N-Dimensional non-abelian dilatonic,stable black holes and their Born-Infeld extension".en_US
dc.identifier.doi10.1007/s10714-009-0835-5
dc.identifier.issn1572-9532 (online)
dc.identifier.issn0001-7701 (online)
dc.identifier.otherDOI: 10.1007/s10714-009-0835-5
dc.identifier.scopus2-s2.0-77950458899
dc.identifier.scopusqualityQ2
dc.identifier.urihttp://dx.doi.org/10.1007/s10714-009-0835-5
dc.identifier.urihttps://hdl.handle.net/11129/2032
dc.identifier.wosWOS:000273852200003
dc.identifier.wosqualityQ2
dc.indekslendigikaynakScopus
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherGeneral Relativity and Gravitation, Springeren_US
dc.relation.ispartofseries;Gen Rel.Grav.42:261-280,2010
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.subjectgravityen_US
dc.subjectgeneral relativityen_US
dc.subjectnon-abelian dilatonicen_US
dc.subjectblack holesen_US
dc.subjectBorn-Infelden_US
dc.titleN-Dimensional non-abelian dilatonic, stable black holes and their Born-Infeld extensionen_US
dc.typeArticle

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