Supersymmetric Rotating Black Hole in a Compactified Spacetime
arXiv:hep-th/0607084 · doi:10.1103/PhysRevD.74.104002
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 (), if the size is small.
7 pages, 3 figures; v2: comparison with black ring removed, detailed discussion of rotation added, refs. added, v3: minor corrections, version to appear in PRD
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Cited by in corpus (7)
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