(2+1)-dimensional dynamical black holes in Einstein-nonlinear Maxwell theory

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dc.authorid0000-0001-9344-5786en_US
dc.authorid0000-0002-7035-6155en_US
dc.contributor.authorGurtug, O.
dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, M.
dc.date.accessioned2024-07-12T21:52:19Z
dc.date.available2024-07-12T21:52:19Z
dc.date.issued2018en_US
dc.departmentMaltepe Üniversitesien_US
dc.description.abstractRadiative extensions of BTZ metric in 2 + 1 dimensions are found which are sourced by nonlinear Maxwell fields and a null current. This may be considered as generalization of the problem formulated long go by Vaidya and Bonnor. The mass and charge are functions of retarded/advanced null coordinate apt for decay/inflation. The new solutions are constructed through a Theorem that works remarkably well for any nonlinear electrodynamic model. Hawking temperature is analyzed for the case of the Born-Infeld electrodynamics.en_US
dc.identifier.doi10.1142/S021773231850027X
dc.identifier.issn0217-7323
dc.identifier.issn1793-6632
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-85041728217en_US
dc.identifier.scopusqualityQ2en_US
dc.identifier.urihttps://dx.doi.org/10.1142/S021773231850027X
dc.identifier.urihttps://hdl.handle.net/20.500.12415/8363
dc.identifier.volume33en_US
dc.identifier.wosWOS:000424737000007en_US
dc.identifier.wosqualityQ2en_US
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoenen_US
dc.publisherWORLD SCIENTIFIC PUBL CO PTE LTDen_US
dc.relation.ispartofMODERN PHYSICS LETTERS Aen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.snmzKY02980
dc.subjectRadiating black holeen_US
dc.subjectEinstein-Power-Maxwell fielden_US
dc.subjectBorn-Infelden_US
dc.title(2+1)-dimensional dynamical black holes in Einstein-nonlinear Maxwell theoryen_US
dc.typeArticle
dspace.entity.typePublication

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