Charged Rotating Black Holes in Higher Dimensions

Details Charged Rotating Black Holes in Higher Dimensions Charged Rotating Black Holes in Higher Dimensions

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.1400k&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Physics

Scientific paper

We consider charged rotating black holes in higher odd dimensions in theories such as Einstein-Maxwell, Einstein-Maxwell-dilaton, and Einstein-Maxwell-Chern-Simons. Retricted to stationary axisymmetric black holes with equal-magnitude angular momenta and a horizon of spherical topology, we present an Ansatz for the metric and the matter fields where the angular dependence is explicitly given and all the unknowns are functions of the radial coordinate only. As a consequence, the field equations reduce to ordinary differential equations. These black holes resemble, in general, their uncharged counterparts, the Myers-Perry black holes. However, when the Chern-Simons term is present new surprising effects appear, such as counterrotation, negative horizon mass, or violation of uniqueness.

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