Seminar series
Date
Tue, 10 Mar 2009
12:00
12:00
Location
L3
Speaker
Akihiro Ishibashi
Organisation
KEK Japan
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.