Post-radiation evolution of black holes

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dc.creatorVilkovisky, G. A.
dc.date2008-03-22
dc.date.accessioned2026-07-07T11:49:18Z
dc.date.available2026-07-07T11:49:18Z
dc.descriptionThe expectation-value equations for the collapse of a macroscopic, spherically symmetric, and uncharged body are integrated up to the limit of validity of semiclassical theory. The collapse finishes with a true stable black hole of the mass microscopically exceeding the vacuum-induced charge. The apparent horizon is almost closed. The most important feature of the solution is the presence of an irremovable Cauchy horizon.
dc.description19 pages, 2 figures. Latex 2.09. Figures PostScript
dc.identifierhttps://arxiv.org/abs/0803.3280
dc.identifierhttp://arxiv.org/abs/0803.3280
dc.identifierPhys.Rev.D77:124043,2008
dc.identifierdoi:10.1103/PhysRevD.77.124043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203184
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePost-radiation evolution of black holes
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