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Stability and thermodynamics of brane black holes

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arxiv gr-qc/0604033 v2 pith:74ECNOCL submitted 2006-04-07 gr-qc astro-phhep-th

E. Abdalla , B. Cuadros-Melgar , A. B. Pavan , C. Molina This is my paper · ORCID
classification gr-qcastro-phhep-th
keywords blackbranescenariosthermodynamicsapplicabilityaxialbekensteinbound
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We consider scalar and axial gravitational perturbations of black hole solutions in brane world scenarios. We show that perturbation dynamics is surprisingly similar to the Schwarzschild case with strong indications that the models are stable. Quasinormal modes and late-time tails are discussed. We also study the thermodynamics of these scenarios verifying the universality of Bekenstein's entropy bound as well as the applicability of 't Hooft's brickwall method.

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Cited by 3 Pith papers

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

  1. Two types of quasinormal modes of Casadio-Fabbri-Mazzacurati brane-world black holes

    gr-qc 2026-02 unverdicted novelty 6.0 of 10

    Quasinormal modes of massive scalars in CFM brane-world black holes split into two types, with modes disappearing at critical masses where real or imaginary frequency parts reach zero.

  2. Geodesic dynamics in brane-de Sitter wormholes

    gr-qc 2025-04 conditional novelty 5.0 of 10

    For an asymptotically de Sitter brane wormhole, the throat is shown to be an unstable fixed point and photon sphere, with a claimed Bogdanov-Takens bifurcation for radial null geodesics.

  3. Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole

    gr-qc 2026-01 unverdicted novelty 4.0 of 10

    Massive scalar perturbations on the Dymnikova regular black hole exhibit growing oscillation frequencies, reduced damping rates leading to quasi-resonances, power-law oscillatory tails, and mass-dependent suppression ...

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