We analytically calculate to leading order the asymptotic form of quasinormal frequencies of Kerr black holes in four, five, and seven dimensions. All the relevant quantities can be explicitly expressed in terms of elliptical integrals. In four dimensions, we confirm the results obtained by Keshest and Hod by comparing the analytic results to the numerical ones.
|期刊||Physical Review D - Particles, Fields, Gravitation and Cosmology|
|出版狀態||已發佈 - 2008 六月 26|
ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)