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

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arxiv gr-qc/0702086 v1 pith:KYHCKBFM submitted 2007-02-15 gr-qc hep-th

Jutta Kunz , Francisco Navarro-Lerida , Eugen Radu This is my paper · ORCID
classification gr-qchep-th
keywords blackholeshorizonrotatinganalyzeangularanti-deapproach
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abstract

We present arguments for the existence of charged, rotating black holes with equal-magnitude angular momenta in an odd number of dimensions $D\geq 5$. 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.

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