On future geodesic completeness for the Einstein-Vlasov system with hyperbolic symmetry

Simple item page
dc.creatorRein, Gerhard
dc.date2002-03-20
dc.date.accessioned2026-07-07T03:26:45Z
dc.date.available2026-07-07T03:26:45Z
dc.descriptionSpacetimes with collisionless matter evolving from data on a compact Cauchy surface with hyperbolic symmetry are shown to be timelike and null geodesically complete in the expanding direction, provided the data satisfy a certain size restriction.
dc.description8 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0203066
dc.identifierhttp://arxiv.org/abs/gr-qc/0203066
dc.identifierMath.Proc.Cambridge Phil.Soc. 137 (2004) 237-244
dc.identifierdoi:10.1017/S0305004103007485
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34167
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn future geodesic completeness for the Einstein-Vlasov system with hyperbolic symmetry
dc.typetext

Files

Collections

arXiv