Cosmological Black Holes on Taub-NUT space in Five-Dimensional Einstein-Maxwell Theory
arXiv:hep-th/0702148 · doi:10.1088/0264-9381/24/13/001
Abstract
The cosmological black hole solution on the Gibbons-Hawking space has been constructed. We also investigate the properties of this solution in the case of a single black hole. Unlike the Kastor-Traschen solution, which becomes static Reissner-Nortström de Sitter solution in a single black hole, this solution is not static even in a single black hole case.
12 pages, 4 figures, some minor corrections, to be published in Classical and Quantum Gravity
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Cited by in corpus (29)
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- Stability of Squashed Kaluza-Klein Black Holes
- Charged Rotating Kaluza-Klein Black Holes Generated by G2(2) Transformation
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- M theory and the Coulomb phase of higher rank DT invariants
- Exact Dynamical Black Hole Solutions in Five or Higher Dimensions
- Reciprocal NUT spacetimes