Einstein-nonlinear Maxwell-Yukawa black hole

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dc.contributor.authorMazharimousavi, S. Habib
dc.contributor.authorHalilsoy, Mustafa
dc.date.accessioned2026-02-06T18:51:41Z
dc.date.issued2019
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractWithin the context of nonlinear electromagnetism, we consider the Yukawa extension of a Reissner-Nordstrom black hole. Exact solution is given which modifies certain characteristics of the latter. Some thermodynamical aspects are given for comparison. The model which is based on a nonpolynomial Lagrangian implicitly may be considered as a useful agent to describe a short-ranged, charged and massive interaction.
dc.identifier.doi10.1142/S0218271819501207
dc.identifier.issn0218-2718
dc.identifier.issn1793-6594
dc.identifier.issue9
dc.identifier.orcid0000-0001-9344-5786
dc.identifier.orcid0000-0002-7035-6155
dc.identifier.scopus2-s2.0-85065325731
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1142/S0218271819501207
dc.identifier.urihttps://hdl.handle.net/11129/15446
dc.identifier.volume28
dc.identifier.wosWOS:000474936500012
dc.identifier.wosqualityQ3
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Modern Physics D
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20260204
dc.subjectYukawa potential
dc.subjectEinstein-Maxwell
dc.subjectexact solution
dc.subjectnonlinear electrodynamics
dc.titleEinstein-nonlinear Maxwell-Yukawa black hole
dc.typeArticle

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