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 | |
| 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