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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=1. The results are extended to j1 for slowly rotating black holes. These modes indicate that the exterior Kerr-Newman geometry is stable in the eikonal approximation.
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Bahram Mashhoon (Tue,) studied this question.
www.synapsesocial.com/papers/6a101d635725bbd5cc608871 — DOI: https://doi.org/10.1103/physrevd.31.290
Bahram Mashhoon
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields
University of Cologne
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