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dc.contributor.author | Fabbri, Alessandro | en_US |
dc.contributor.author | Pérez Cañellas, Armando | en_US |
dc.date.accessioned | 2008-12-10T12:29:18Z | - |
dc.date.available | 2008-12-10T12:29:18Z | - |
dc.date.issued | 2007-03-12 | en_US |
dc.identifier.citation | Physical Review D 75: 064009 (2007) | en_US |
dc.identifier.issn | 1550-7998 | en_US |
dc.identifier.uri | http://hdl.handle.net/10261/9141 | - |
dc.description | 4 pages, 1 figure.-- PACS nrs.: 04.70.Dy; 03.67.-a.-- ISI Article Identifier: 000245333600044.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-th/0611152 | en_US |
dc.description.abstract | We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a matter-radiation thermalization hypothesis on the Black Hole interior, which translates into a particular entangled state with thermal Schmidt coefficients. We investigate the consequences of this proposal for matter entering the horizon, as described by a Canonical density matrix characterized by the matter temperature T. The emitted radiation is explicitly calculated and is shown to follow a thermal spectrum with an effective temperature T-eff. We analyze the evaporation process in the quasistatic approximation, highlighting important differences in the late stages with respect to the usual semiclassical evolution, and calculate the fidelity of the emitted Hawking radiation relative to the infalling matter. | en_US |
dc.description.sponsorship | This work has been supported by the Spanish Grants AYA2004-08067-C01, FPA2005-00711, FIS2005-05736-C03-03, the EU Network MRTN-CT-2004-005104 and by Generalitat Valenciana (Grant No. GV05/264). | - |
dc.format.extent | 2373 bytes | - |
dc.format.mimetype | text/plain | - |
dc.language.iso | eng | en_US |
dc.publisher | American Physical Society | en_US |
dc.rights | openAccess | en_US |
dc.subject | [PACS] Quantum aspects of black holes, evaporation, thermodynamics | - |
dc.subject | [PACS] Quantum information | - |
dc.title | Black hole evaporation in a thermalized final-state projection model | en_US |
dc.type | artículo | en_US |
dc.identifier.doi | 10.1103/PhysRevD.75.064009 | - |
dc.description.peerreviewed | Peer reviewed | en_US |
dc.relation.publisherversion | http://dx.doi.org/10.1103/PhysRevD.75.064009 | en_US |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.openairetype | artículo | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
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Fabbri_Perez_PRD_75_064009_2007.pdf | 97,82 kB | Adobe PDF | Visualizar/Abrir |
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