Quasinormal Modes in three-dimensional time-dependent Anti-de Sitter spacetime
arXiv:gr-qc/0307097 · doi:10.1088/0256-307X/21/3/003
Abstract
The massless scalar wave propagation in the time-dependent BTZ black hole background has been studied. It is shown that in the quasi-normal ringing both the decay and oscillation time-scales are modified in the time-dependent background.
8 pages and 7 figures
References in corpus (20)
- The Black Hole in Three Dimensional Space Time
- Quasi-Normal Modes of Stars and Black Holes
- Late-Time Behavior of Stellar Collapse and Explosions: I. Linearized Perturbations
- The (2+1)-Dimensional Black Hole
- Scalar, electromagnetic and Weyl perturbations of BTZ black holes: quasi normal modes
- Wave Propagation in Gravitational Systems: Late Time Behavior
- Scalar Wave Falloff in Asymptotically Anti-de Sitter Backgrounds
- Quasinormal modes of Reissner-Nordstrm Anti-de Sitter Black Holes
- Late Time Tail of Wave Propagation on Curved Spacetime
- Telling Tails In The Presence Of A Cosmological Constant
- Comments on Black Holes in String Theory
- Radiative falloff in Schwarzschild-de Sitter spacetime
- Evolving of a massless scalar field in Reissner--Nordström Anti--de Sitter spacetimes
- Scalar wave propagation in topological black hole backgrounds
- Asymptotic power-law tails of massive scalar fields in Reissner-Nordström background
- Late-time evolution of a self-interacting scalar field in the spacetime of dilaton black hole
- Object picture of quasinormal ringing on the background of small Schwarzschild Anti-de Sitter black holes
- Support of dS/CFT correspondence from perturbations of three dimensional spacetime
- Wave Tails in Time Dependent Backgrounds
- Numerical simulation of the massive scalar field evolution in the Reissner-Nordström black hole background