Quasinormal modes of d-dimensional spherical black holes with a near extreme cosmological constant

Abstract

We derive an expression for the quasinormal modes of scalar perturbations in near extreme d-dimensional Schwarzschild-de Sitter and Reissner-Nordstrom-de Sitter black holes. We show that, in the near extreme limit, the dynamics of the scalar field is characterized by a Poschl-Teller effective potential. The results are qualitatively independent of the spacetime dimension and field mass.

5 pages, REVTeX4, version to be published in Physical Review D

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