Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2003-09-02
Phys.Rev. D68 (2003) 124017
Physics
High Energy Physics
High Energy Physics - Theory
13 pages, 2 figures, several references are added
Scientific paper
10.1103/PhysRevD.68.124017
We find the gravitational resonance (quasinormal) modes of the higher dimensional Schwarzschild and Reissner-Nordstrem black holes. The effect on the quasinormal behavior due to the presence of the $\lambda$ term is investigated. The QN spectrum is totally different for different signs of $\lambda$. In more than four dimensions there excited three types of gravitational modes: scalar, vector, and tensor. They produce three different quasinormal spectra, thus the isospectrality between scalar and vector perturbations, which takes place for D=4 Schwarzschild and Schwarzschild-de-Sitter black holes, is broken in higher dimensions. That is the scalar-type gravitational perturbations, connected with deformations of the black hole horizon, which damp most slowly and therefore dominate during late time of the black hole ringing.
No associations
LandOfFree
Gravitational quasinormal radiation of higher-dimensional black holes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gravitational quasinormal radiation of higher-dimensional black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational quasinormal radiation of higher-dimensional black holes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-493650