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A uniqueness theorem for charged rotating black holes in five- dimensional minimal supergravity
Abstract
We show that a charged rotating black hole in five-dimensional Einstein-Maxwell-Chern-Simons theory is uniquely characterized by the mass, charge, and two independent angular momenta, under the assumptions of the existence of two commuting axial isometries and spherical topology of horizon cross-sections. Therefore, such a black hole must be described by the Chong-Cveti\v{c}-L\"u-Pope metric.