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.

arXiv comment5 pages. To appear in Phys. Rev. D

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