Quasinormal modes of Reissner-Nordstrom black holes

Details Quasinormal modes of Reissner-Nordstrom black holes Quasinormal modes of Reissner-Nordstrom black holes

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..41.2986l&link_type=abstract

Physical Review D - Particles and Fields, 3rd Series (ISSN 0556-2821), vol. 41, May 15, 1990, p. 2986-2997.

Statistics

Computation

63

Black Holes (Astronomy), Gravitational Waves, Reissner-Nordstrom Solution, Schwarzschild Metric, Wave Equations, Computational Astrophysics, Partial Differential Equations, Perturbation Theory

Scientific paper

A matrix-eigenvalue algorithm is presented for accurately computing the quasi-normal frequencies and modes of charged static blackholes. The method is then refined through the introduction of a continued-fraction step. The approach should generalize to a variety of nonseparable wave equations, including the Kerr-Newman case of charged rotating blackholes.

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