Schwarzschild black-hole normal modes using the Hill determinant

Details Schwarzschild black-hole normal modes using the Hill determinant Schwarzschild black-hole normal modes using the Hill determinant

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvd..40.2568m&link_type=abstract

Physical Review D (Particles and Fields), Volume 40, Issue 8, 15 October 1989, pp.2568-2571

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18

Scientific paper

The quasinormal modes of the black hole have been determined by solving
the linearized perturbation equation by using a series solution, derived
earlier, and the Hill determinant. This proves a useful method for
determining such frequencies. These are quoted and compared with those
obtained by other numerical and semianalytical methods.

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