Object picture of quasinormal ringing on the background of small Schwarzschild Anti-de Sitter black holes
Preprint
- 6 February 2001
Abstract
We investigated the evolution of a scalar field propagating in small Schwarzschild Anti-de Sitter black holes. The imaginary part of the quasinormal frequency decreases with the horizon size and the real part of the quasinormal frequency keeps nearly as a constant. The object-picture clarified the question on the quasinormal modes for small Anti-de Sitter black holes. Dependence of quasinormal modes on spacetime dimensions and the multipole index for small Anti-de Sitter black holes have also been illustrated.Keywords
All Related Versions
- Version 1, 2001-01-19, ArXiv
- Version 2, 2001-02-06, ArXiv
- Published version: Physical Review D, 63 (12).
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