### 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≡a/G4M=1), if the size is small.

Original language | English |
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Article number | 104002 |

Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |

Volume | 74 |

Issue number | 10 |

DOIs | |

Publication status | Published - 2006 Nov 7 |

### ASJC Scopus subject areas

- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)

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## Cite this

Maeda, K. I., Ohta, N., & Tanabe, M. (2006). Supersymmetric rotating black hole in a compactified spacetime.

*Physical Review D - Particles, Fields, Gravitation and Cosmology*,*74*(10), [104002]. https://doi.org/10.1103/PhysRevD.74.104002