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.

Original languageEnglish
Pages (from-to)2387-2400
Number of pages14
JournalGeneral Relativity and Gravitation
Volume44
Issue number9
DOIs
StatePublished - Sep 2012
Externally publishedYes

Keywords

  • Classical stability
  • Quasinormal modes
  • de Sitter spacetime

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