MG12 - Talk detail
 

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Abstract

Black Holes in Einstein-Maxwell-Chern-Simons Theory

I shall present a new Kerr-Schild type framework for rotating charged black holes in five-dimensional minimal gauged supergravity, or equivalently in the Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant and with the Chern-Simons coefficient equal to unity. This framework ensures the simple derivation of the general solution of Chong, Cvetic, Lu and Pope for nonextremal rotating charged black holes in five-dimensional minimal gauged supergravity. Next, assuming the Kerr-Schild-type framework as an ansatz, I shall discuss new analytic solutions for slowly rotating charged AdS black holes in the Einstein-Maxwell-Chern-Simons theory with any value of the Chern-Simons coefficient.

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