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

J. Podolsky·J. B. Griffiths
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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.

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J. Podolsky, J. B. Griffiths. 2006-01-30. Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time. https://doi.org/10.1103/physrevd.73.044018

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