Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9855043 | Nuclear Physics B | 2005 | 24 Pages |
Abstract
Using the Pöshl-Teller approximation, we evaluate the neutrino quasinormal modes (QNMs) of a Kerr-Newman-de Sitter black hole. The result shows that for a Kerr-Newman-de Sitter black hole, massless neutrino perturbation of large Î, positive m and small value of n will decay slowly.
Related Topics
Physical Sciences and Engineering
Mathematics
Mathematical Physics
Authors
Jia-Feng Chang, You-Gen Shen,