Gravitational collapse in loop quantum gravity

dc.creatorModesto, Leonardo
dc.date2006-10-14
dc.date.accessioned2026-07-07T11:26:31Z
dc.date.available2026-07-07T11:26:31Z
dc.descriptionIn this paper we study the gravitational collapse in loop quantum gravity. We consider the space-time region inside the Schwarzschild black hole event horizon and we divide this region in two parts, the first one where the matter (dust matter) is localized and the other (outside) where the metric is Kantowski-Sachs type. We calculate the state solving Hamiltonian constraint and we obtain a set of three difference equations that give a regular and natural evolution beyond the classical singularity point in "r=0" localized.
dc.description16 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0610074
dc.identifierhttp://arxiv.org/abs/gr-qc/0610074
dc.identifierInt.J.Theor.Phys.47:357-373,2008
dc.identifierdoi:10.1007/s10773-007-9458-3
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195848
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational collapse in loop quantum gravity
dc.typetext

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