Quasi-normal modes of a black hole

Details Quasi-normal modes of a black hole Quasi-normal modes of a black hole

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.136..251p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 136, no. 2, Aug. 1987, p. 251-257.

Statistics

Computation

3

Black Holes (Astronomy), Computational Astrophysics, Amplitudes, Perturbation, Polynomials, Schwarzschild Metric

Scientific paper

The quasi-normal modes of a black hole are calculated requiring that the
ingoing amplitudes vanish at inifinity. The amplitude is obtained by
making the solutions valid close to and far away from the horizon. The
normal modes are obtained in the form of polynomial solutions.

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