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Gravitational quasinormal modes for Kerr anti-de Sitter black holes

Lookup NU author(s): Mr M Giannatteo Giammatteo, Professor Ian Moss

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Abstract

We investigate the quasinormal modes for gravitational perturbations of rotating black holes in four-dimensional anti-de Sitter (AdS) spacetime. The study of the quasinormal frequencies related to these modes is relevant to the AdS/CFT correspondence. Although results have been obtained for Schwarzschild and Reissner-Nordstrom AdS black holes, quasinormal frequencies of Kerr-AdS black holes are computed for the first time. We solve the Teukolsky equations in AdS spacetime, providing a second-order and a Padé approximation for the angular eigenvalues associated with the Teukolsky angular equation. The transformation theory and the Regge-Wheeler-Zerilli equations for Kerr-AdS are obtained. ©2005 IOP Publishing Ltd.


Publication metadata

Author(s): Giammatteo M, Moss IG

Publication type: Article

Publication status: Published

Journal: Classical and Quantum Gravity

Year: 2005

Volume: 22

Issue: 9

Pages: 1803-1824

ISSN (print): 0264-9381

ISSN (electronic): 1361-6382

Publisher: Institute of Physics Publishing Ltd.

URL: http://dx.doi.org/10.1088/0264-9381/22/9/021

DOI: 10.1088/0264-9381/22/9/021


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