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Although finding numerically the quasinormal modes of a nonrotating black hole is a well-studied question, the physics of the problem is often hidden behind complicated numerical procedures aimed at avoiding the direct solution of the spectral system in this case.
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Schutz B. F., Centrella J., Cutler C., Hughes S. A
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Pani P., Berti E., Cardoso V., Chen Y., Norte R
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