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dc.contributor.authorAmir, M.-
dc.contributor.authorAli, M. D.-
dc.contributor.authorMaharaj, S. D.-
dc.date.accessioned2021-06-12T10:18:27Z-
dc.date.available2021-06-12T10:18:27Z-
dc.date.issued2021-06-12-
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1801-
dc.description.abstractWe derive a rotating counterpart of the five-dimensional electrically charged Bardeen regular black holes spacetime by employing the Giampieri algorithm on static one. The associated nonlinear electrodynamics source is computed in order to justify the rotating solution. We thoroughly discuss the energy conditions and the other properties of the rotating spacetime. The black hole thermodynamics of the rotating spacetime is also presented. In particular, the thermodynamic quantities such as the Hawking temperature and the heat capacity are calculated and plotted to see the thermal behavior. The Hawking temperature profile of the black hole implies that the regular black holes are thermally colder than its singular counterpart. On the other hand, we find that the heat capacity has two branches: the negative branch corresponds to the unstable phase and the positive branch corresponds to that of the stable phase for a suitable choice of the physical parameters characterizing the black holes.en_US
dc.language.isoen_USen_US
dc.subjectblack holesen_US
dc.subjectmodified gravityen_US
dc.subjectblack hole thermodynamicsen_US
dc.titleRotating five-dimensional electrically charged bardeen regular black holesen_US
dc.typeArticleen_US
Appears in Collections:Year-2020

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