Charged Rotating Black Holes on DGP Brane
arXiv:0711.1074 · doi:10.1142/S0217751X09045479
Abstract
We consider charged rotating black holes localized on a three-brane in the DGP model. Assuming a -symmetry across the brane and with a stationary and axisymmetric metric ansatz on the brane, a particular solution is obtained in the Kerr-Schild form. This solution belongs to the accelerated branch of the DGP model and has the characteristic of the Kerr-Newman-de Sitter type solution in general relativity. Using a modified version of Boyer-Lindquist coordinates we examine the structures of the horizon and ergosphere.
LaTeX, 15 pages, Discussion on a bulk solution is added
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