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.
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schutz1993classicalgeneralized Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors N Andersson,M E Araujo,B F Schutz, N Andersson, M E Araujo, B F Schutz
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Journal classical and quantum gravity
Year 1993
DOI
10.1088/0264-9381/10/4/010
URL
https://sciprofiles.com/publication/view/b10eaf4dc1bfa3e62771faaff06e8120
Keywords
black hole normal modes

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