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, focusing on black holes with a single angular momentum, and with two equal-magnitude angular momenta.
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