Rotating Black Holes in Higher Dimensions

Abstract

The properties of higher-dimensional black holes can differ significantly from those of black holes in four dimensions, since neither the uniqueness theorem, nor the staticity theorem or the topological censorship theorem generalize to higher dimensions. We first discuss black holes of Einstein-Maxwell theory and Einstein-Maxwell-Chern-Simons theory with spherical horizon topology. Here new types of stationary black holes are encountered. We then discuss nonuniform black strings and present evidence for a horizon topology changing transition.

Small errors corrected

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Cited by in corpus (16)

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• `Hidden' Symmetries of Higher Dimensional Rotating Black Holes
• Analytic solutions of the geodesic equation in higher dimensional static spherically symmetric space-times
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• Extremal vacuum black holes in higher dimensions
• Generalized Killing-Yano equations in D=5 gauged supergravity
• Black Holes in Higher-Dimensional Gravity
• G2 Dualities in D=5 Supergravity and Black Strings
• Quasilocal formalism and thermodynamics of asymptotically flat black objects
• Separability of the massive Dirac's equation in 5-dimensional Myers-Perry black hole geometry and its relation to a rank-three Killing-Yano tensor
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• Generating technique for $U(1{)}^{3}5D$ supergravity
• Rotating black holes with equal-magnitude angular momenta in d=5 Einstein-Gauss-Bonnet theory
• Symmetry operators and separability of massive Klein-Gordon and Dirac equations in the general 5-dimensional Kerr-(anti-)de Sitter black hole background
• Charged-Rotating Black Holes in Higher-dimensional (A)DS-Gravity
• Particle Dynamics Around the Black String