Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12323/7413
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dc.contributor.authorPourhassan, Behnam-
dc.contributor.authorFarahani, Hoda-
dc.contributor.authorKazemian, Farideh-
dc.contributor.authorSakallı, İzzet-
dc.contributor.authorUpadhyay, Sudhaker-
dc.contributor.authorSingh, Dharm Veer-
dc.date.accessioned2024-03-28T07:50:07Z-
dc.date.available2024-03-28T07:50:07Z-
dc.date.issued2024-
dc.identifier.urihttp://hdl.handle.net/20.500.12323/7413-
dc.description.abstractIn this paper, we use the holographic principle to obtain a modified metric of black holes that reproduces the exponentially corrected entropy. The exponential correction of the black hole entropy comes from non-perturbative corrections. It interprets as a quantum effect which affects black hole thermodynamics especially in the infinitesimal scales. Hence, it may affect black hole stability at the final stage. Then, we study modified thermodynamics due to the non-perturbative corrections and calculate thermodynamics quantities of several non-rotating black holes.en_US
dc.language.isoenen_US
dc.publisherPhysics of the Dark Universeen_US
dc.relation.ispartofseriesVol. 44;-
dc.subjectNon-perturbative correctionen_US
dc.subjectQuantum nature of black holeen_US
dc.subjectStabilityen_US
dc.titleNon-perturbative correction on the black hole geometryen_US
dc.typeArticleen_US
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