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Quasinormal modes of the near extremal Schwarzschild-de Sitter black hole

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arxiv gr-qc/0301078 v2 pith:ZHOZJRAN submitted 2003-01-21 gr-qc hep-phhep-th

classification gr-qchep-phhep-th
keywords extremalmodesnearquasinormalblackholesitterapproximation
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We present an exact expression for the quasinormal modes of scalar, electromagnetic and gravitational perturbations of a near extremal Scwarzschild-de Sitter black hole and we show why a previous approximation holds exactly in this near extremal regime. In particular, our results give the asymptotic behavior of the quasinormal frequencies for highly damped modes, which as recently attracted much attention due to the proposed identification of its real part with the Barbero-Immirzi parameter.

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Cited by 7 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Quasinormal modes of Proca and Maxwell fields in $d$-dimensional Schwarzschild-AdS black holes

    gr-qc 2026-05 conditional novelty 7.0 of 10

    Scalar-type Maxwell perturbations in large d≥5 Schwarzschild-AdS black holes exhibit purely imaginary low-frequency quasinormal modes, confirmed numerically and by asymptotic matching.

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    gr-qc 2026-07 accept novelty 6.0 of 10

    Spectral Method yields the complete QNM spectrum (fundamentals, overtones, overdamped modes) of the Bonanno-Reuter black hole, missed by prior WKB analyses.

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    gr-qc 2025-06 conditional novelty 6.0 of 10

    Purely imaginary gravitational quasinormal modes of Reissner-Nordström-de Sitter black holes are computed and shown to obey a universal small-hole formula and to generate late-time exponential tails.

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    hep-th 2025-06 conditional novelty 4.0 of 10

    Graviton quasinormal modes reproduce only the bulk part of the one-loop determinant on S^2 x S^2; the residual edge character is isolated but its lower-spin interpretation is not derived.

  7. Massive scalar field perturbations of 4D de Sitter Einstein-Gauss-Bonnet black holes

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    Massive scalar perturbations of 4D Einstein-Gauss-Bonnet de Sitter black holes are stable and show three quasinormal mode branches, including a non-perturbative de Sitter branch that disappears in the Schwarzschild-de...

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