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Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/212
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dc.contributor.authorBurić, Majaen
dc.contributor.authorRadovanović, Vojaen
dc.date.accessioned2022-07-05T16:30:31Z-
dc.date.available2022-07-05T16:30:31Z-
dc.date.issued2001-01-01en
dc.identifier.issn0556-2821en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/212-
dc.description.abstractIn this paper we analyze the quantum correction for a Schwarzschild black hole in the Unruh state in the framework of the spherically symmetric gravity (SSG) model. SSG is a two-dimensional dilaton model that is obtained by spherically symmetric reduction from four-dimensional theory. We find the one-loop geometry of the (anti)evaporating black hole and corrections for mass, entropy, and apparent horizon. ©2001 The American Physical Society.en
dc.relation.ispartofPhysical Review Den
dc.titleQuantum corrections for an (anti) evaporating black holeen
dc.typeArticleen
dc.identifier.doi10.1103/PhysRevD.63.044020en
dc.identifier.scopus2-s2.0-0035076552en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0035076552en
dc.relation.issue4en
dc.relation.volume63en
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
crisitem.author.orcid0000-0002-4383-633X-
crisitem.author.orcid0000-0003-0675-1836-
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