Kerr-Schild Method and Geodesic Structure in Codimension-2 Brane Black Holes
General Relativity and Quantum Cosmology
2014-11-20 v3 High Energy Physics - Theory
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.
Keywords
Cite
@article{arxiv.0912.0218,
title = {Kerr-Schild Method and Geodesic Structure in Codimension-2 Brane Black Holes},
author = {Bertha Cuadros-Melgar and Susana Aguilar and Nelson Zamorano},
journal= {arXiv preprint arXiv:0912.0218},
year = {2014}
}
Comments
30 pages, 9 figures. One new reference added. Published version in Phys. Rev. D