Radiative spacetimes approaching the Vaidya metric

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dc.creatorPodolsky, Jiri
dc.creatorSvitek, Otakar
dc.date2005-06-03
dc.date.accessioned2026-07-07T03:29:46Z
dc.date.available2026-07-07T03:29:46Z
dc.descriptionWe analyze a class of exact type II solutions of the Robinson-Trautman family which contain pure radiation and (possibly) a cosmological constant. It is shown that these spacetimes exist for any sufficiently smooth initial data, and that they approach the spherically symmetric Vaidya-(anti-)de Sitter metric. We also investigate extensions of the metric, and we demonstrate that their order of smoothness is in general only finite. Some applications of the results are outlined.
dc.description12 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0506016
dc.identifierhttp://arxiv.org/abs/gr-qc/0506016
dc.identifierPhys.Rev. D71 (2005) 124001
dc.identifierdoi:10.1103/PhysRevD.71.124001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35306
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRadiative spacetimes approaching the Vaidya metric
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