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Supersymmetric Rotating Black Hole in a Compactified Spacetime

Kei-ichi Maeda·Nobuyoshi Ohta·Makoto Tanabe
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Abstract

We construct a supersymmetric rotating black hole with asymptotically flat four-dimensional spacetime times a circle, by superposing an infinite number of BMPV black hole solutions at the same distance in one direction. The near horizon structure is the same as that of the five-dimensional BMPV black hole. The rotation of this black hole can exceed the Kerr bound in general relativity ($q\equiv a/G_4 M=1$), if the size is small.

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Kei-ichi Maeda, Nobuyoshi Ohta, Makoto Tanabe. 2006-10-30. Supersymmetric Rotating Black Hole in a Compactified Spacetime. https://doi.org/10.1103/physrevd.74.104002

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