Generalized Einstein-Power Maxwell theory in 2+1-dimensions

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dc.contributor.authorAmirabi, Z.
dc.date.accessioned2026-02-06T18:51:31Z
dc.date.issued2021
dc.departmentDoğu Akdeniz Üniversitesi
dc.description.abstractUsing the generalized Einstein-Power Maxwell Lagrangian which has been proposed very recently by Mazharimousavi (Class Quantum Gravity 37:197001, 2020), we find an electric black hole solution in 2+1-dimensions. The solution is singular and non-asymptotically flat associated with only one horizon. The thermodynamic properties are investigated, and it is shown that the black hole is thermally stable. In the context of the extended thermodynamic phase space, we find Smarr's formula consistent with the first law of the black holes.
dc.identifier.doi10.1140/epjp/s13360-021-01575-w
dc.identifier.issn2190-5444
dc.identifier.issue5
dc.identifier.scopus2-s2.0-85106940435
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1140/epjp/s13360-021-01575-w
dc.identifier.urihttps://hdl.handle.net/11129/15377
dc.identifier.volume136
dc.identifier.wosWOS:000657681200001
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/closedAccess
dc.snmzKA_WoS_20260204
dc.subjectRotating Black Branes
dc.subjectHoles
dc.subjectThermodynamics
dc.subjectSupergravity
dc.subjectEnergy
dc.titleGeneralized Einstein-Power Maxwell theory in 2+1-dimensions
dc.typeArticle

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