Black holes in loop quantum gravity: the complete space-time

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dc.creatorGambini, Rodolfo
dc.creatorPullin, Jorge
dc.date2008-05-08
dc.date.accessioned2026-07-07T11:50:38Z
dc.date.available2026-07-07T11:50:38Z
dc.descriptionWe consider the quantization of the complete extension of the Schwarzschild space-time using spherically symmetric loop quantum gravity. We find an exact solution corresponding to the semi-classical theory. The singularity is eliminated but the space-time still contains a horizon. Although the solution is known partially numerically and therefore a proper global analysis is not possible, a global structure akin to a singularity-free Reissner--Nordström space-time including a Cauchy horizon is suggested.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0805.1187
dc.identifierhttp://arxiv.org/abs/0805.1187
dc.identifierPhys.Rev.Lett.101:161301,2008
dc.identifierdoi:10.1103/PhysRevLett.101.161301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/203622
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleBlack holes in loop quantum gravity: the complete space-time
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