Quasinormal modes in Schwarschild black holes due to arbitrary spin fields
| dc.creator | Shu, Fu-Wen | |
| dc.creator | Shen, You-Gen | |
| dc.date | 2005-01-30 | |
| dc.date | 2005-05-31 | |
| dc.date.accessioned | 2026-07-07T10:48:17Z | |
| dc.date.available | 2026-07-07T10:48:17Z | |
| dc.description | 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. | |
| dc.description | 11 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0501098 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0501098 | |
| dc.identifier | Phys.Lett.B619:340-346,2005 | |
| dc.identifier | doi:10.1016/j.physletb.2005.05.077 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183826 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Quasinormal modes in Schwarschild black holes due to arbitrary spin fields | |
| dc.type | text |