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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3576
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dc.contributor.authorAshtekar, A.-
dc.contributor.authorTaveras, Victor-
dc.contributor.authorVaradarajan, Madhavan-
dc.date.accessioned2008-06-28T10:58:14Z-
dc.date.available2008-06-28T10:58:14Z-
dc.date.issued2008-05-
dc.identifier.citationPhysical Review Letters, 2008, Vol.100, 211302en
dc.identifier.issn1550-2368(online)-
dc.identifier.issn1550-7998 (print)-
dc.identifier.urihttp://hdl.handle.net/2289/3576-
dc.descriptionOpen Access.en
dc.description.abstractWe analyze Hawking evaporation of the Callan-Giddings-Harvey-Strominger black holes from a quantum geometry perspective and show that information is not lost, primarily because the quantum space-time is sufficiently larger than the classical. Using suitable approximations to extract physics from quantum space-times we establish that (i) the future null infinity of the quantum space-time is sufficiently long for the past vacuum to evolve to a pure state in the future, (ii) this state has a finite norm in the future Fock space, and (iii) all the information comes out at future infinity; there are no remnants.en
dc.format.extent310942 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevLett.100.211302en
dc.relation.urihttp://arxiv.org/abs/0801.1811en
dc.rights2008 The American Physical Societyen
dc.titleInformation is not lost in the evaporation of 2D black holesen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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