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Five-Dimensional Charged Rotating Black Holes

Jutta Kunz·Francisco Navarro-Lerida·Anna Katinka Petersen
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Abstract

We consider charged rotating black holes in 5-dimensional Einstein-Maxwell theory. These black holes are asymptotically flat, they possess a regular horizon of spherical topology and two independent angular momenta associated with two distinct planes of rotation. We discuss their global and horizon properties, and derive a generalized Smarr formula. We construct these black holes numerically, focussing on black holes with a single angular momentum, and with two equal-magnitude angular momenta.

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Jutta Kunz, Francisco Navarro-Lerida, Anna Katinka Petersen. 2005-03-02. Five-Dimensional Charged Rotating Black Holes. https://doi.org/10.1016/j.physletb.2005.03.056

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