Kerr black-hole quasinormal frequencies

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 67, Issue 8, 2003, Pages

  Hod, Shahar ^a  

^a WEIZMANN INSTITUTE OF SCIENCE   (Israel)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; BOHR EFFECT; GRAVITY; OSCILLATION; QUANTUM MECHANICS;

EID: 1842463859     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.081501     Document Type: Article

References (33)

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33. Note that in the Schwarzschild case with (Formula presented) there is a sharp transition from the behavior of the first few QNM frequencies into the regular asymptotic behavior, which occurs at the 10th overtone (see Fig. 11 of 9). Thus, one should not necessarily go to the (Formula presented) limit in order to obtain a fairly good estimate of the asymptotic behavior.