Supersymmetric Rotating Black Hole in a Compactified Spacetime
High Energy Physics - Theory
2009-11-11 v3
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.
Keywords
Cite
@article{arxiv.hep-th/0607084,
title = {Supersymmetric Rotating Black Hole in a Compactified Spacetime},
author = {Kei-ichi Maeda and Nobuyoshi Ohta and Makoto Tanabe},
journal= {arXiv preprint arXiv:hep-th/0607084},
year = {2009}
}
Comments
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