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

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preprint
posted on 03.02.2006, 11:19 by J. Podolsky, Jerry Griffiths
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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School

  • Science

Department

  • Mathematical Sciences

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152797 bytes

Publication date

2006

Notes

This is a pre-print. It is also available at: http://xxx.soton.ac.uk/abs/gr-qc/0601130.

Language

en

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