Electromagnetic quasinormal modes of D-dimensional black holes II
arXiv:0706.2933 · doi:10.1007/s10714-007-0538-8
Abstract
By using the sixth order WKB approximation we calculate for an electromagnetic field propagating in D-dimensional Schwarzschild and Schwarzschild de Sitter black holes its quasinormal frequencies for the fundamental mode and first overtones. We study the dependence of these QN frequencies on the value of the cosmological constant and the spacetime dimension. We also compare with the known results for the gravitational perturbations propagating in the same background. Moreover we exactly compute the QN frequencies of the electromagnetic field propagating in D-dimensional massless topological black hole and for charged D-dimensional Nariai spacetime we exactly calculate the QN frequencies of the coupled electromagnetic and gravitational perturbations.
34 pages, 14 figures, 6 tables
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Cited by in corpus (8)
- Stability of higher dimensional Reissner-Nordstrom-anti-de Sitter black holes
- Looking at the Gregory-Laflamme instability through quasi-normal modes
- A comparative study of Dirac quasinormal modes of charged black holes in higher dimensions
- Quasinormal Modes for Dynamical Black Holes
- Electromagnetic quasinormal modes of an asymptotically Lifshitz black hole
- Entropy spectrum of the D-dimensional massless topological black hole
- Echoes of axial gravitational perturbations in stars of uniform density
- Gravitons on Nariai Edges