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Paper detail

Rotating Black Holes in Higher Dimensions with a Cosmological Constant

We present the metric for a rotating black hole with a cosmological constant and with arbitrary angular momenta in all higher dimensions. The metric is given in both Kerr-Schild and Boyer-Lindquist form. In the Euclidean-signature case, we also obtain smooth compact Einstein spaces on associated S^{D-2} bundles over S^2, infinitely many for each odd D\ge 5. Applications to string theory and M-theory are indicated.

preprint2004arXivOpen access
G. W. GibbonsH. LuD. N. PageC. N. Pope
hep-th
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G. W. GibbonsH. LuD. N. PageC. N. Pope

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