Kerr-Schild Method and Geodesic Structure in Codimension-2 Brane Black Holes
arXiv:0912.0218 · doi:10.1103/PhysRevD.81.126010
Abstract
We consider the black hole solutions of five-dimensional gravity with a Gauss-Bonnet term in the bulk and an induced gravity term on a 2-brane of codimension-2. Applying the Kerr-Schild method we derive additional solutions which include charge and angular momentum. To improve our understanding of this geometry we study the geodesic structure of such spacetimes.
30 pages, 9 figures. One new reference added. Published version in Phys. Rev. D
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