Cosmological Black Holes on Taub-NUT space in Five-Dimensional Einstein-Maxwell Theory
Daisuke Ida, Hideki Ishihara, Masashi Kimura, Ken Matsuno, Yoshiyuki, Morisawa, Shinya Tomizawa
TL;DR
This paper constructs a cosmological black hole solution on Gibbons-Hawking space within five-dimensional Einstein-Maxwell theory, revealing non-static properties even for a single black hole, differing from known static solutions.
Contribution
It introduces a new cosmological black hole solution on Gibbons-Hawking space that remains non-static in the single black hole case, expanding understanding of such configurations.
Findings
The solution is not static for a single black hole.
It differs from the Kastor-Traschen solution.
Properties of the solution are analyzed in detail.
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-Nortstr\"om de Sitter solution in a single black hole, this solution is not static even in a single black hole case.
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