Rotating Braneworld Black Holes
Astrophysics
2007-05-23 v1
Abstract
We present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black holes with a tidal charge in the Randall-Sundrum braneworld. The tidal charge appears as an imprint of nonlocal gravitational effects from the bulk space. We also discuss the physical properties of these black holes and their possible astrophysical appearance.
Cite
@article{arxiv.astro-ph/0612735,
title = {Rotating Braneworld Black Holes},
author = {Alikram N. Aliev},
journal= {arXiv preprint arXiv:astro-ph/0612735},
year = {2007}
}
Comments
To appear in the Proceedings of the Eleventh Marcel Grossmann Meeting, Berlin, Germany, 23-29 Jule 2006, 3pp., World Scientific, Singapore (2007)