Supersymmetric rotating black hole in a compactified spacetime

Kei Ichi Maeda; Nobuyoshi Ohta; Makoto Tanabe

doi:10.1103/PhysRevD.74.104002

Supersymmetric rotating black hole in a compactified spacetime

Kei Ichi Maeda^*, Nobuyoshi Ohta, Makoto Tanabe

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

10 Citations (Scopus)

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
Article number	104002
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	74
Issue number	10
DOIs	https://doi.org/10.1103/PhysRevD.74.104002
Publication status	Published - 2006
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.74.104002

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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≡a/G4M=1), if the size is small.",

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AU - Ohta, Nobuyoshi

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AB - 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.

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ER -

Supersymmetric rotating black hole in a compactified spacetime

Abstract

ASJC Scopus subject areas

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