Non-Abelian magnetic black strings versus black holes

dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, M.
dc.date.accessioned2026-02-06T18:51:29Z
dc.date.issued2016
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWe present d+1-dimensional pure magnetic Yang-Mills (YM) black strings (or 1-branes) induced by the d-dimensional Einstein-Yang-Mills-Dilaton black holes. The Born-Infeld version of the YM field makes our starting point which goes to the standard YM field through a limiting procedure. The lifting from black holes to black strings (with less number of fields) is done by adding an extra, compact coordinate. This amounts to the change of horizon topology from Sd-2 to a product structure. Our black string in 5 dimensions is a rather special one, with uniform Hawking temperature and non-asymptotically flat structure. As the YM charge becomes large the string gets thinner to tend into a breaking point and transform into a 4-dimensional black hole.
dc.identifier.doi10.1140/epjp/i2016-16138-y
dc.identifier.issn2190-5444
dc.identifier.issue5
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.scopus2-s2.0-85007211706
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjp/i2016-16138-y
dc.identifier.urihttps://hdl.handle.net/11129/15350
dc.identifier.volume131
dc.identifier.wosWOS:000375679300002
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherSpringer Heidelberg
dc.relation.ispartofEuropean Physical Journal Plus
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.titleNon-Abelian magnetic black strings versus black holes
dc.typeArticle

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