Publication Date:
2011-08-19
Description:
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.
Keywords:
ASTROPHYSICS
Type:
Physical Review D - Particles and Fields, 3rd Series (ISSN 0556-2821); 41; 2986-299
Format:
text
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