Phenomenological loop quantum geometry of the Schwarzschild black hole

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dc.creatorChiou, Dah-Wei
dc.date2008-07-04
dc.date2008-09-10
dc.date.accessioned2026-07-07T11:52:16Z
dc.date.available2026-07-07T11:52:16Z
dc.descriptionThe interior of a Schwarzschild black hole is investigated at the level of phenomenological dynamics with the discreteness corrections of loop quantum geometry implemented in two different improved quantization schemes. In one scheme, the classical black hole singularity is resolved by the quantum bounce, which bridges the black hole interior with a white hole interior. In the other scheme, the classical singularity is resolved and the event horizon is also diffused by the quantum bounce. Jumping over the quantum bounce, the black hole gives birth to a baby black hole with a much smaller mass. This lineage continues as each classical black hole brings forth its own descendant in the consecutive classical cycle, giving the whole extended spacetime fractal structure, until the solution eventually descends into deep Planck regime, signaling a breakdown of the semiclassical description. The issues of scaling symmetry and no-hair theorem are also discussed.
dc.description26 pages, 6 figures, 1 table; version to appear in PRD
dc.identifierhttps://arxiv.org/abs/0807.0665
dc.identifierhttp://arxiv.org/abs/0807.0665
dc.identifierPhys.Rev.D78:064040,2008
dc.identifierdoi:10.1103/PhysRevD.78.064040
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204173
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePhenomenological loop quantum geometry of the Schwarzschild black hole
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