期刊
PHYSICS LETTERS B
卷 639, 期 3-4, 页码 362-367出版社
ELSEVIER
DOI: 10.1016/j.physletb.2006.06.066
关键词
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We consider charged rotating black holes of Einstein-Maxwell theory in D = 2N + 1 dimensions, D >= 5. These black holes are asymptotically flat and possess a regular horizon of spherical topology. While they generically possess N independent angular momenta, associated with N distinct planes of rotation, we here focus on black holes with equal-magnitude angular momenta. In that case the angular dependence can be treated explicitly, and the field equations reduce to a system of 5 ordinary differential equations, which depend on the dimension. We solve these equations numerically in D = 5, 7 and 9 dimensions. We discuss the global and horizon properties of these black holes, as well as their extremal limits. (c) 2006 Elsevier B.V. All rights reserved.
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