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On the quasinormal modes of the de Sitter spacetime

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Abstract

Modifying a method by Horowitz and Hubeny for asymptotically anti-de Sitter black holes, we establish the classical stability of the quasinormal modes of the de Sitter spacetime. Furthermore using a straightforward method we calculate the de Sitter quasinormal frequencies of the gravitational perturbations and discuss some properties of the radial functions of these quasinormal modes.

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Authors and Affiliations

  1. Centro de Investigación en Ciencia Aplicada y Tecnología Avanzada, Unidad Legaria, Instituto Politécnico Nacional, Calzada Legaria # 694. Colonia Irrigación. Delegación Miguel Hidalgo, Mexico, DF, 11500, Mexico

    A. López-Ortega

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  1. A. López-Ortega
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Correspondence to A. López-Ortega.

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López-Ortega, A. On the quasinormal modes of the de Sitter spacetime. Gen Relativ Gravit 44, 2387–2400 (2012). https://doi.org/10.1007/s10714-012-1398-4

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