Classical instability of Kerr-AdS black holes and the issue of final state

Details Classical instability of Kerr-AdS black holes and the issue of final state Classical instability of Kerr-AdS black holes and the issue of final state

2006-07-22

arxiv.org/abs/hep-th/0607162v2

Phys.Rev. D74 (2006) 044008

Physics

High Energy Physics

High Energy Physics - Theory

11 pages, RevTex4. v2: small typos corrected. Version to appear in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.74.044008

It is now established that small Kerr-Anti-de Sitter (Kerr-AdS) black holes are unstable against scalar perturbations, via superradiant amplification mechanism. We show that small Kerr-AdS black holes are also unstable against gravitational perturbations and we compute the features of this instability. We also describe with great detail the evolution of this instability. In particular, we identify its endpoint state. It corresponds to a Kerr-AdS black hole whose boundary is an Einstein universe rotating with the light velocity. This black hole is expected to be slightly oblate and to co-exist in equilibrium with a certain amount of outside radiation.

Affiliated with

Also associated with

No associations

Rating

Classical instability of Kerr-AdS black holes and the issue of final state does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Classical instability of Kerr-AdS black holes and the issue of final state, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Classical instability of Kerr-AdS black holes and the issue of final state will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-301096