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Model of black hole evolution

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dc.contributor.authorRusso, J. G. (Jorge Guillermo)cat
dc.date.accessioned2010-05-06T12:03:05Z
dc.date.available2010-05-06T12:03:05Z
dc.date.issued1996cat
dc.description.abstractWe investigate a model where the quantum dynamics of black hole evaporation is determined by imposing a boundary on the apparent horizon with suitable boundary conditions. An unconventional scenario for the evolution emerges: only an insignificant fraction of energy of order (mG)-1 is radiated out; the outgoing wave carries a very small part of the quantum-mechanical information of the collapsed body, the bulk of the information remaining in the final stable black hole geometry.eng
dc.format.extent7 p.cat
dc.format.mimetypeapplication/pdfeng
dc.identifier.idgrec512112cat
dc.identifier.issn0556-2821cat
dc.identifier.urihttps://hdl.handle.net/2445/12473
dc.language.isoengeng
dc.publisherThe American Physical Societyeng
dc.relation.isformatofReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.55.871cat
dc.relation.ispartofPhysical Review D, 1996, vol. 55, núm 2, p. 871-877cat
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.55.871
dc.rights(c) The American Physical Society, 1996
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationRelativitat general (Física)cat
dc.subject.classificationGravitaciócat
dc.subject.classificationForats negres (Astronomia)cat
dc.subject.otherGeneral relativity (Physics)eng
dc.subject.otherGravitacióeng
dc.subject.otherBlack holes (Astronomy)eng
dc.titleModel of black hole evolutioneng
dc.typeinfo:eu-repo/semantics/articleeng
dc.typeinfo:eu-repo/semantics/publishedVersion

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