Speaker
panapol kanjanaphomchom
Description
Abstract
The quasinormal modes(qnm) of a massless charged scalar field in the 3+1 dimensional anti de Sitter(AdS) Reissener-Nordstrom(RN) spacetime are analytically calculated. The solutions of the scale field under the influence of the RN black hole are approximated by satisfying the boundary conditions at the horizon and the far away zone from the black hole. Our result for the small black hole mass is consistent with the numerical result.
Keywords: Quasinormal modes, Quasinormal frequencies, AdS black holes, Reissener-Nordrom black holes
