Radiating black hole solutions in arbitrary dimensions

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dc.creatorGhosh, S. G.
dc.creatorDawood, A. K.
dc.date2008-01-28
dc.date.accessioned2026-07-07T11:55:37Z
dc.date.available2026-07-07T11:55:37Z
dc.descriptionWe prove a theorem that characterizes a large family of non-static solutions to Einstein equations in $N$-dimensional space-time, representing, in general, spherically symmetric Type II fluid. It is shown that the best known Vaidya-based (radiating) black hole solutions to Einstein equations, in both four dimensions (4D) and higher dimensions (HD), are particular cases from this family. The spherically symmetric static black hole solutions for Type I fluid can also be retrieved. A brief discussion on the energy conditions, singularities and horizons is provided.
dc.descriptionRevTeX 9 pages, no figures
dc.identifierhttps://arxiv.org/abs/0801.4342
dc.identifierhttp://arxiv.org/abs/0801.4342
dc.identifierGen.Rel.Grav.40:9-21,2008
dc.identifierdoi:10.1007/s10714-007-0511-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205303
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRadiating black hole solutions in arbitrary dimensions
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