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

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

2006-01-30

arxiv.org/abs/gr-qc/0601130v1

Phys.Rev. D73 (2006) 044018

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages. To appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.73.044018

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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