期刊
PHYSICAL REVIEW LETTERS
卷 93, 期 17, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.93.171102
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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 the Boyer-Lindquist form. In the Euclidean-signature case, we also obtain smooth compact Einstein spaces on associated SD-2 bundles over S-2, infinitely many for each odd Dgreater than or equal to5. Applications to string theory and M-theory are indicated.
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