Phys. Rev. D 73, 044018 (2006) [5 pages]Accelerating Kerr–Newman black holes in (anti-)de Sitter space-timeReceived 22 November 2005; published 15 February 2006 A class of exact solutions of the Einstein–Maxwell equations is presented which describes an accelerating and rotating charged black hole in an asymptotically de Sitter or anti-de Sitter universe. The metric is presented in a new and convenient form in which the meaning of the parameters is clearly identified, and from which the physical properties of the solution can readily be interpreted. © 2006 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.73.044018
DOI:
10.1103/PhysRevD.73.044018
PACS:
04.20.Jb, 04.30.Nk, 04.70.Bw
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