Cho, H. T.; Cornell, A. S.; Doukas, Jason; Naylor, Wade Black hole quasinormal modes using the asymptotic iteration method. (English) Zbl 1197.83065 Classical Quantum Gravity 27, No. 15, Article ID 155004, 12 p. (2010). Summary: We show that the asymptotic iteration method (AIM) allows one to numerically find the quasinormal modes of Schwarzschild and Schwarzschild de Sitter black holes. An added benefit of the method is that it can also be used to calculate the Schwarzschild anti-de Sitter quasinormal modes for the case of spin-zero perturbations. We also discuss an improved version of the AIM, more suitable for numerical implementation. Cited in 18 Documents MSC: 83C57 Black holes 83-08 Computational methods for problems pertaining to relativity and gravitational theory 83C25 Approximation procedures, weak fields in general relativity and gravitational theory Keywords:singular perturbations; turning point theory; WKB methods; black holes; space-time singularities; cosmic censorship; gravitational waves PDFBibTeX XMLCite \textit{H. T. Cho} et al., Classical Quantum Gravity 27, No. 15, Article ID 155004, 12 p. (2010; Zbl 1197.83065) Full Text: DOI arXiv