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

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.

5 pages. To appear in Phys. Rev. D

References in corpus (1)

• Radiation from accelerated black holes in an anti-de Sitter universe

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