Boost-rotation symmetric spacetimes - review

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dc.creatorPravda, V.
dc.creatorPravdova, A.
dc.date2000-03-16
dc.date.accessioned2026-07-07T11:46:14Z
dc.date.available2026-07-07T11:46:14Z
dc.descriptionBoost-rotation symmetric spacetimes are the only locally asymptotically flat axially symmetric electrovacuum spacetimes with a further symmetry that are radiative. They are realized by uniformly accelerated particles of various kinds or black holes. Their general properties are summarized. Several examples of boost-rotation symmetric solutions of the Maxwell and Einstein equations are studied: uniformly accelerated electric and magnetic multipoles, the Bonnor-Swaminarayan solutions, the C-metric and the spinning C-metric.
dc.description30 pages, 11 eps figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0003067
dc.identifierhttp://arxiv.org/abs/gr-qc/0003067
dc.identifierCzech.J.Phys.50:333-376,2000
dc.identifierdoi:10.1023/A:1022862309863
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202156
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBoost-rotation symmetric spacetimes - review
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