Stability of charged rotating black holes in the eikonal approximation

Details Stability of charged rotating black holes in the eikonal approximation Stability of charged rotating black holes in the eikonal approximation

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvd..31..290m&link_type=abstract

Physical Review D (Particles and Fields), Volume 31, Issue 2, 15 January 1985, pp.290-293

Physics

34

Black Holes

Scientific paper

The stability of the exterior Kerr-Newman spacetime to high-frequency perturbations is investigated. The complex frequencies associated with the oscillations of a charged rotating black hole are determined for the perturbation angular momentum parameters j=||m||>>1. The results are extended to j>=||m||>>1 for slowly rotating black holes. These modes indicate that the exterior Kerr-Newman geometry is stable in the eikonal approximation.

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