Hairy extension of the Bertotti-Robinson spacetime in the Einstein-Maxwell-scalar theory is a black hole in closed spatial geometries

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dc.contributor.authorMazharimousavi, S. Habib
dc.date.accessioned2026-02-06T18:47:45Z
dc.date.issued2022
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn analogy with the Einstein-Maxwell-Dilaton black hole which is a hairy extension of the Reissner-Nordstrom black hole, we introduce a hairy extension for the Bertotti-Robinson spacetime in the context of the Einstein-Maxwell-scalar theory. The new spacetime is a closed S (3) black hole powered by a pure magnetic field. The energy-momentum tensor is an anisotropic fluid-like form such that p(r)/rho and p(perpendicular to)/rho are u (the radial coordinate)-dependent and at the horizon becomes -1/3 1/3
dc.identifier.doi10.1088/1361-6382/ac8141
dc.identifier.issn0264-9381
dc.identifier.issn1361-6382
dc.identifier.issue16
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.scopus2-s2.0-85137201879
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1088/1361-6382/ac8141
dc.identifier.urihttps://hdl.handle.net/11129/14537
dc.identifier.volume39
dc.identifier.wosWOS:000843827300001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIop Publishing Ltd
dc.relation.ispartofClassical and Quantum Gravity
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectEinstein-Maxwell-scalar
dc.subjectblack hole
dc.subjectBertotti-Robinson
dc.subjectMisner-Sharp
dc.titleHairy extension of the Bertotti-Robinson spacetime in the Einstein-Maxwell-scalar theory is a black hole in closed spatial geometries
dc.typeArticle

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