Generalized Bohr-Sommerfeld formula for Schwarzschild black hole normal modes
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ID: 274019
1993
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Abstract
A generalized Bohr-Sommerfeld-type formula determining the quasinormal-mode frequencies of Schwarzschild black holes is derived using the phase-integral method with three transition points. The formula is valid provided that these points are well separated from each other, and is remarkably accurate for the high-overtone modes. It makes a great improvement over the conventional Bohr-Sommerfeld formula, derived from two transition points.
| Reference Key |
schutz1993classicalgeneralized
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| Authors | N Andersson,M E Araujo,B F Schutz;N Andersson;M E Araujo;B F Schutz; |
| Journal | classical and quantum gravity |
| Year | 1993 |
| DOI |
10.1088/0264-9381/10/4/010
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