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

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

C. Molina
(
- Sao Paulo U.
)

Apr, 2003

5 pages

Published in:

Phys.Rev.D 68 (2003) 064007

e-Print:

gr-qc/0304053 [gr-qc]

DOI:

10.1103/PhysRevD.68.064007

Report number:

1565-2003

View in:

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Abstract: (arXiv)

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.

04.70.Bw
04.30.Nk
black hole: oscillation
any-dimensional
symmetry: sphere
black hole: Schwarzschild
black hole: Reissner-Nordstroem
space-time: de Sitter
effective potential

References(33)

Figures(0)

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