Quasinormal Modes and Hidden Conformal Symmetry of Warped dS Black Hole
arXiv:1110.3991 · doi:10.1103/PhysRevD.84.124039
Abstract
In this paper, we analytically calculate the quasinormal modes of scalar, vector, tensor, and spinor perturbations of the warped dS black hole. There are two horizons for the warped dS black hole, namely, the black hole horizon and the cosmological horizon . In the calculation, we impose the ingoing boundary condition at the black hole horizon and the outgoing boundary condition at the cosmological horizon. We also investigate the hidden conformal symmetry of the warped dS black hole in the region between the black hole horizon and the cosmological horizon . We use the hidden conformal symmetry to construct the quasinormal modes in an algebraic way and find that the results agree with the analytically ones. It turns out that the frequencies of the quasinormal modes could be identified with the poles in the thermal boundary-boundary correlators.
26 pages, references added, published version
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Cited by in corpus (8)
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- Quasinormal Modes of Bardeen Black Hole: Scalar Perturbations
- Thermodynamics of Black Hole Horizons and Kerr/CFT Correspondence
- Aspects of Warped AdS/CFT Correspondence
- Regular black holes in de Sitter universe: scalar field perturbations and quasinormal modes
- Accelerating BTZ spacetime
- On emergent conformal symmetry near the photon ring
- Notes on Self-dual Warped dS Spacetime