Consistent Loop Quantum Cosmology

Simple item page
dc.creatorBojowald, Martin
dc.date2008-11-25
dc.date.accessioned2026-07-07T12:56:48Z
dc.date.available2026-07-07T12:56:48Z
dc.descriptionA consistent combination of quantum geometry effects rules out a large class of models of loop quantum cosmology and their critical densities as they have been used in the recent literature. In particular, the critical density at which an isotropic universe filled with a free, massless scalar field would bounce must be well below the Planck density. In the presence of anisotropy, no model of the Schwarzschild black hole interior analyzed so far is consistent.
dc.description13 pages
dc.identifierhttps://arxiv.org/abs/0811.4129
dc.identifierhttp://arxiv.org/abs/0811.4129
dc.identifierClass.Quant.Grav.26:075020,2009
dc.identifierdoi:10.1088/0264-9381/26/7/075020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224707
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleConsistent Loop Quantum Cosmology
dc.typetext

Files

Collections

arXiv