The Bianchi IX model in Loop Quantum Cosmology

dc.creatorBojowald, Martin
dc.creatorDate, Ghanashyam
dc.creatorHossain, Golam Mortuza
dc.date2004-04-08
dc.date.accessioned2026-07-07T03:28:35Z
dc.date.available2026-07-07T03:28:35Z
dc.descriptionThe Bianchi IX model has been used often to investigate the structure close to singularities of general relativity. Its classical chaos is expected to have, via the BKL scenario, implications even for the approach to general inhomogeneous singularities. Thus, it is a popular model to test consequences of modifications to general relativity suggested by quantum theories of gravity. This paper presents a detailed proof that modifications coming from loop quantum gravity lead to a non-chaotic effective behavior. The way this is realized, independently of quantization ambiguities, suggests a new look at initial and final singularities.
dc.description41 pages, 3 figures, revtex4
dc.identifierhttps://arxiv.org/abs/gr-qc/0404039
dc.identifierhttp://arxiv.org/abs/gr-qc/0404039
dc.identifierClass.Quant.Grav. 21 (2004) 3541-3570
dc.identifierdoi:10.1088/0264-9381/21/14/015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34884
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleThe Bianchi IX model in Loop Quantum Cosmology
dc.typetext

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