An Extensive Search for Overtones in Schwarzschild Black Holes
arXiv:gr-qc/0611023 · doi:10.1590/S0103-97332007000300018
Abstract
In this paper we show that with standard methods it is possible to obtain highly precise results for QNMs. In particular, secondary modes are obtained by numerical integration. We compare several results making a detailed analysis.
2 figures, revtex4 used