Accelerating Kerr–Newman black holes in (anti-)de Sitter space-time

J. Podolský and J. B. Griffiths
Phys. Rev. D 73, 044018 – Published 15 February 2006

Abstract

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.

  • Received 22 November 2005

DOI:https://doi.org/10.1103/PhysRevD.73.044018

©2006 American Physical Society

Authors & Affiliations

J. Podolský1 and J. B. Griffiths2

  • 1Institute of Theoretical Physics, Faculty of Mathematics and Physics, Charles University in Prague, V Holešovičkách 2, 18000 Prague 8, Czech Republic
  • 2Department of Mathematical Sciences, Loughborough University, Loughborough, Leics. LE11 3TU, United Kingdom

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Issue

Vol. 73, Iss. 4 — 15 February 2006

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