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Accelerating Kerr-Newman black holes in (anti-) de Sitter space-time
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...
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| Main Authors: | , |
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| Format: | Default Preprint |
| Published: |
2006
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| Subjects: | |
| Online Access: | https://hdl.handle.net/2134/744 |
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