Quasi-normal modes of a black hole localized on a codimension-two brane of finite tension
arXiv:0708.3363 · doi:10.1103/PhysRevD.76.104031
Abstract
We calculate the quasi-normal modes of black holes localized on a 3-brane of finite tension embedded in six-dimensional flat spacetime. Using the WKB approximation, we obtain the frequencies of various types of perturbation both analytically and numerically for arbitrary brane tension. We thus extend earlier analytical results which were derived for a brane of small tension.
17 pages, uses bibTeX, 5 figures
References in corpus (5)
- Quasi-Normal Modes of Brane-Localised Standard Model Fields
- Quasi-Normal Modes of Brane-Localised Standard Model Fields II: Kerr Black Holes
- Stability and thermodynamics of brane black holes
- Evaporation of a black hole off of a tense brane
- Wave dynamics of a six-dimensional black hole localized on a tensional three-brane
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- Stability of higher dimensional Reissner-Nordstrom-anti-de Sitter black holes
- Looking at the Gregory-Laflamme instability through quasi-normal modes
- Greybody Factors for Rotating Black Holes on Codimension-2 Branes
- Bulk dominated fermion emission on a Schwarzschild background
- Black Holes on Thin 3-branes of Codimension-2 and their Extension into the Bulk
- Bulk scalar emission from a rotating black hole pierced by a tense brane
- Fermion excitations of a tense brane black hole
- Quasinormal modes of black holes localized on the Randall-Sundrum 2-brane
- Particle emission from a black hole on a tense codimension-2 brane
- Evolution of Massive Scalar Fields in the Spacetime of a Tense Brane Black Hole
- Fermion evaporation of a black hole off a tense brane
- Codimension-2 black hole solutions on a thin 3-brane and their extension into the bulk