Cosmological Black Holes on Taub-NUT space in Five-Dimensional Einstein-Maxwell Theory
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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
12 pages, 4 figures, some minor corrections, to be published in Classical and Quantum Gravity