| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9861115 | Physics Letters B | 2005 | 7 Pages |
Abstract
The Newman-Penrose formalism is used to deal with the massless scalar, neutrino, electromagnetic, gravitino and gravitational quasinormal modes (QNMs) in Schwarzschild black holes in a united form. The quasinormal mode frequencies evaluated by using the 3rd-order WKB potential approximation show that the boson perturbations and the fermion perturbations behave in a contrary way for the variation of the oscillation frequencies with spin, while this is no longer true for the damping's, which variate with s in a same way both for boson and fermion perturbations.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Fu-Wen Shu, You-Gen Shen,