We are investigating singularity structure of the rotating black hole and naked singularity spacetimes in the Randall-Sundrum second type (RSII) of the brane-world scenario. We will show that structure of this singularity is very similar to its classical counterpart, even in the cases of negative tidal charge, which is equivalent to the Kerr-Newman black hole with the complex charge Q (with zero real part). We also study behaviour of the ergosphere and will show that this region can exists under specific situation.
Proceedings of RAGtime 14-16: Workshops on black holes and neutron stars
- Pub Date:
- December 2014
- Randall Sundrum;