Journal
GENERAL RELATIVITY AND GRAVITATION
Volume 44, Issue 9, Pages 2387-2400Publisher
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10714-012-1398-4
Keywords
de Sitter spacetime; Quasinormal modes; Classical stability
Funding
- CONACYT Mexico
- SNI Mexico
- EDI-IPN
- COFAA-IPN
- [SIP-20120773]
- [SIP-20121648]
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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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