Quasinormal modes of Dirac field perturbation in Reissner-Nordström black hole surrounded by quintessence
arXiv:0910.5128
Abstract
The dirac quasinormal modes of the Reissner-Nordström black hole surrounded by quintessence are investigated using the third WKB approximation. We find that the magnitude of the imaginary part of the quasinormal mode frequencies increases firstly and then decreases as the charge increases, but it decreases as the absolute value of increases. The magnitude of the imaginary part of quasinormal complex frequencies is smaller than those with no quintessence. That is to say, the dirac field damps more slowly due to the presence of quintessence.
12pages, 11 figures