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 language | English |
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Pages (from-to) | 2387-2400 |
Number of pages | 14 |
Journal | General Relativity and Gravitation |
Volume | 44 |
Issue number | 9 |
DOIs | |
State | Published - Sep 2012 |
Externally published | Yes |
Keywords
- Classical stability
- Quasinormal modes
- de Sitter spacetime