Generalized Bohr-Sommerfeld formula for Schwarzschild black hole normal modes
Clicks: 104
ID: 274019
1993
Article Quality & Performance Metrics
Overall Quality
Improving Quality
0.0
/100
Combines engagement data with AI-assessed academic quality
Reader Engagement
Emerging Content
3.6
/100
12 views
12 readers
Trending
AI Quality Assessment
Not analyzed
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
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; |
| Journal | classical and quantum gravity |
| Year | 1993 |
| DOI |
10.1088/0264-9381/10/4/010
|
| URL | |
| Keywords |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.