Stability of the Schwarzschild Interior in Loop Quantum Gravity

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dc.creatorBoehmer, Christian G.
dc.creatorVandersloot, Kevin
dc.date2008-07-18
dc.date2008-08-14
dc.date.accessioned2026-07-07T11:44:56Z
dc.date.available2026-07-07T11:44:56Z
dc.descriptionIn recent work, the Schwarzschild interior of a black hole was investigated, incorporating quantum gravitational modifications due to loop quantum gravity. The central Schwarzschild singularity was shown to be replaced by a Nariai type universe. In this brief report we show that this interior solution is stable with respect to small perturbations, in contrast to the classical Nariai universe.
dc.description4 pages, 4 figures; references added, minor modifications
dc.identifierhttps://arxiv.org/abs/0807.3042
dc.identifierhttp://arxiv.org/abs/0807.3042
dc.identifierPhys.Rev.D78:067501,2008
dc.identifierdoi:10.1103/PhysRevD.78.067501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201724
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleStability of the Schwarzschild Interior in Loop Quantum Gravity
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