Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvl..52.1361f&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 52, April 16, 1984, p. 1361-1364.
Astronomy and Astrophysics
Astronomy
52
Black Holes (Astronomy), Oscillations, Rotating Matter, Circular Orbits, Damping, Perturbation
Scientific paper
A new analytic method for the determination of quasinormal oscillations of a black hole is presented. It is based on a connection between the quasinormal modes and the bound states of the inverted black-hole potentials. With use of this method, the quasinormal frequencies of a Schwarzschild, a Reissner-Nordström, and a slowly rotating Kerr black hole are determined in the eikonal approximation. Moreover, the authors provide evidence for the stability of an extreme Kerr black hole.
Ferrari Valeria
Mashhoon Bahram
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