Black hole quasinormal modes using the asymptotic iteration method

Details Black hole quasinormal modes using the asymptotic iteration method Black hole quasinormal modes using the asymptotic iteration method

2009-12-15

arxiv.org/abs/0912.2740v3

Class.Quant.Grav.27:155004,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, LaTeX; references added; substantially expanded version

Scientific paper

10.1088/0264-9381/27/15/155004

In this article we show that the asymptotic iteration method (AIM) allows one to numerically find the quasinormal modes of Schwarzschild and Schwarzschild de Sitter (SdS) black holes. An added benefit of the method is that it can also be used to calculate the Schwarzschild anti-de Sitter (SAdS) quasinormal modes for the case of spin zero perturbations. We also discuss an improved version of the AIM, more suitable for numerical implementation.

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