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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24037
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dc.contributor.authorSchuetzhold, Ralf-
dc.contributor.authorMaia, Clovis-
dc.date.accessioned2014-05-20T14:08:40Z-
dc.date.accessioned2016-10-25T17:14:39Z-
dc.date.available2014-05-20T14:08:40Z-
dc.date.available2016-10-25T17:14:39Z-
dc.date.issued2008-04-25-
dc.identifierhttp://dx.doi.org/10.1088/1751-8113/41/16/164065-
dc.identifier.citationJournal of Physics A-mathematical and Theoretical. Bristol: Iop Publishing Ltd, v. 41, n. 16, p. 6, 2008.-
dc.identifier.issn1751-8113-
dc.identifier.urihttp://hdl.handle.net/11449/24037-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24037-
dc.description.abstractUsing a kink of arbitrary shape as a toy model for a black hole ( horizon), we study the back-reaction of the evaporation process and find that the horizon is always pushed back ( as in the gravitational case). The associated heat capacity and entropy variation, on the other hand, can be positive or negative, depending on the parameters.en
dc.format.extent6-
dc.language.isoeng-
dc.publisherIop Publishing Ltd-
dc.sourceWeb of Science-
dc.titleBlack-hole back-reaction - a toy modelen
dc.typeoutro-
dc.contributor.institutionTech Univ Dresden-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationTech Univ Dresden, Inst Theoret Phys, D-01062 Dresden, Germany-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.doi10.1088/1751-8113/41/16/164065-
dc.identifier.wosWOS:000254778400066-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofJournal of Physics A: Mathematical and Theoretical-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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