Black hole quasinormal modes using the asymptotic iteration method

H. T. Cho; A. S. Cornell; Jason Doukas; Wade Naylor

doi:10.1088/0264-9381/27/15/155004

Black hole quasinormal modes using the asymptotic iteration method

H. T. Cho, A. S. Cornell, Jason Doukas, Wade Naylor

Research output: Contribution to journal › Article › peer-review

102 Citations (Scopus)

Abstract

In this paper 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.

Original language	English
Article number	155004
Journal	Classical and Quantum Gravity
Volume	27
Issue number	15
DOIs	https://doi.org/10.1088/0264-9381/27/15/155004
Publication status	Published - 2010
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1088/0264-9381/27/15/155004

Cite this

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title = "Black hole quasinormal modes using the asymptotic iteration method",

abstract = "In this paper 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.",

author = "Cho, \{H. T.\} and Cornell, \{A. S.\} and Jason Doukas and Wade Naylor",

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AU - Cho, H. T.

AU - Cornell, A. S.

AU - Doukas, Jason

AU - Naylor, Wade

PY - 2010

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N2 - In this paper 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.

AB - In this paper 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.

UR - https://www.scopus.com/pages/publications/77953737357

U2 - 10.1088/0264-9381/27/15/155004

DO - 10.1088/0264-9381/27/15/155004

M3 - Article

AN - SCOPUS:77953737357

SN - 0264-9381

VL - 27

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 15

M1 - 155004

ER -

Black hole quasinormal modes using the asymptotic iteration method

Abstract

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