Slow-rotating dirty black hole in Einstein-nonlinear electrodynamics-dilaton theory

dc.contributor.authorMazharimousavi, S. Habib
dc.date.accessioned2026-02-06T18:37:43Z
dc.date.issued2024
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractIn this study, we aim to obtain a slow-rotating black hole in the theory of gravity coupled to square- root nonlinear electrodynamics and a dilaton scalar field. Its static and spherically symmetric version has been recently found in EPJC83(2023)406 which is a 2-parameter non-asymptotically flat black hole with a singularity located at its center. In its slow-rotating version, the solution is a three-parameter black hole that is also non-asymptotically flat and singular at its center. The electric field up to the first order of the rotation parameter is uniform in analogy with its static counterpart.
dc.identifier.doi10.1016/j.dark.2024.101696
dc.identifier.issn2212-6864
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.scopus2-s2.0-85206698861
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1016/j.dark.2024.101696
dc.identifier.urihttps://hdl.handle.net/11129/12580
dc.identifier.volume46
dc.identifier.wosWOS:001340669300001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherElsevier
dc.relation.ispartofPhysics of the Dark Universe
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectDirty black hole
dc.subjectHairy black hole
dc.subjectSquare-root model
dc.subjectMaxwell-dilaton
dc.subjectUniform electric field
dc.subjectBlack hole
dc.titleSlow-rotating dirty black hole in Einstein-nonlinear electrodynamics-dilaton theory
dc.typeArticle

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