Abstract
Boost-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.
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Pravda, V., Pravdová, A. Boost-rotation symmetric spacetimes – Review. Czechoslovak Journal of Physics 50, 333–375 (2000). https://doi.org/10.1023/A:1022862309863
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DOI: https://doi.org/10.1023/A:1022862309863