Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time
General Relativity and Quantum Cosmology
2009-11-11 v1
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.
Keywords
Cite
@article{arxiv.gr-qc/0601130,
title = {Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time},
author = {J. Podolsky and J. B. Griffiths},
journal= {arXiv preprint arXiv:gr-qc/0601130},
year = {2009}
}
Comments
5 pages. To appear in Phys. Rev. D