Higher dimensional rotating black holes in Einstein-Maxwell theory with negative cosmological constant

Abstract

We present arguments for the existence of charged, rotating black holes with equal-magnitude angular momenta in an odd number of dimensions $D\ge 5$. These solutions posses a regular horizon of spherical topology and approach asymptotically the Anti-de Sitter spacetime background. We analyze their global charges, their gyromagnetic ratio and their horizon properties.

11 pages, 8 figures

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