Radiation equations for black holes

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dc.creatorVilkovisky, G. A.
dc.date2005-11-18
dc.date.accessioned2026-07-07T11:06:20Z
dc.date.available2026-07-07T11:06:20Z
dc.descriptionIt has been shown in the previous paper that the metric in the semiclassical region of the collapse spacetime is expressed purely kinematically through the Bondi charges. Here the Bondi charges are expressed through this metric by calculating the vacuum radiation against its background. The result is closed equations for the metric and the Bondi charges. Notably, there is a nonvanishing flux of the vacuum-induced matter charge.
dc.description16 pages, 1 figure. Latex 2.09. Figure PNG
dc.identifierhttps://arxiv.org/abs/hep-th/0511183
dc.identifierhttp://arxiv.org/abs/hep-th/0511183
dc.identifierPhys.Lett.B634:456-464,2006
dc.identifierdoi:10.1016/j.physletb.2006.02.012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/189484
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRadiation equations for black holes
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