Robinson-Trautman spacetimes in higher dimensions

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dc.creatorPodolsky, Jiri
dc.creatorOrtaggio, Marcello
dc.date2006-05-26
dc.date.accessioned2026-07-07T07:09:45Z
dc.date.available2026-07-07T07:09:45Z
dc.descriptionAs an extension of the Robinson-Trautman solutions of D=4 general relativity, we investigate higher dimensional spacetimes which admit a hypersurface orthogonal, non-shearing and expanding geodesic null congruence. Einstein's field equations with an arbitrary cosmological constant and possibly an aligned pure radiation are fully integrated, so that the complete family is presented in closed explicit form. As a distinctive feature of higher dimensions, the transverse spatial part of the general line element must be a Riemannian Einstein space, but it is otherwise arbitrary. On the other hand, the remaining part of the metric is - perhaps surprisingly - not so rich as in the standard D=4 case, and the corresponding Weyl tensor is necessarily of algebraic type D. While the general family contains (generalized) static Schwarzschild-Kottler-Tangherlini black holes and extensions of the Vaidya metric, there is no analogue of important solutions such as the C-metric.
dc.description11 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0605136
dc.identifierhttp://arxiv.org/abs/gr-qc/0605136
dc.identifierClass.Quant.Grav. 23 (2006) 5785-5797
dc.identifierdoi:10.1088/0264-9381/23/20/002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111191
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleRobinson-Trautman spacetimes in higher dimensions
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