Charged Rotating Kaluza-Klein Black Holes in Five Dimensions

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We construct a new charged rotating Kaluza-Klein black hole solution in the five-dimensional Einstein-Maxwell theory with a Chern-Simon term. The features of the solutions are also investigated. The spacetime is asymptotically locally flat, i.e., it asymptotes to a twisted $\rm S^1$ bundle over the four-dimensional Minkowski spacetime. The solution describe a non-BPS black hole rotating in the direction of the extra dimension. The solutions have the limits to the supersymmetric black hole solutions, a new extreme non-BPS black hole solutions and a new rotating non-BPS black hole solution with a constant twisted $\rm S^1$ fiber.
18 pages, 4 figures

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High Energy Physics - Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/205076

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0801.0164
 http://arxiv.org/abs/0801.0164
 Phys.Rev.D77:044040,2008
 doi:10.1103/PhysRevD.77.044040

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arXiv