Stability and thermodynamics of brane black holes

Abstract

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.

arXiv comment13 pages, 8 figures, published version

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• Hawking radiation in a Rotating Kaluza-Klein Black Hole with Squashed Horizons
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• Wave dynamics of a six-dimensional black hole localized on a tensional three-brane
• Evolution of Brane-Localised Standard Model Fields in Gauss-Bonnet theory
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• Scalar perturbations and quasi-normal modes of a non-linear magnetic-charged black hole surrounded by quintessence
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• Wormholes in de Sitter branes
• Overtones of black holes via time-domain integration
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• Strong Gravitational Lensing in a Charged Squashed Kaluza- Klein Black hole
• Physical Properties of Brane-World Black Hole Solutions via a Confining Potential
• Strong Gravitational Lensing in a Charged Squashed Kaluza- Klein Gödel Black hole
• Telling late-time tails for a massive scalar field in the background of brane-localized black holes
• Quasi-normal modes of a black hole localized on a codimension-two brane of finite tension
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• BTZ Solutions on Codimension-2 Braneworlds
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