Supersymmetric Rotating Black Hole in a Compactified Spacetime

Details Supersymmetric Rotating Black Hole in a Compactified Spacetime Supersymmetric Rotating Black Hole in a Compactified Spacetime

2006-07-13

arxiv.org/abs/hep-th/0607084v3

Phys.Rev. D74 (2006) 104002

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, 3 figures; v2: comparison with black ring removed, detailed discussion of rotation added, refs. added, v3: minor corr

Scientific paper

10.1103/PhysRevD.74.104002

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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