Quasi-Normal Modes and Exponential Energy Decay for the Kerr-de Sitter Black Hole

Author:

Dyatlov Semyon

Publisher

Springer Science and Business Media LLC

Subject

Mathematical Physics,Statistical and Nonlinear Physics

Reference38 articles.

1. Aguilar J., Combes J.M.: A class of analytic perturbations for one-body Schrödinger Hamiltonians. Commun. Math. Phys 22, 269–279 (1971)

2. Andersson, L., Blue, P.: Hidden symmetries and decay for the wave equation on the Kerr spacetime, http://arxiv.org/abs/0908.2265v2 [math.Ap], 2009

3. Bachelot A.: Gravitational scattering of electromagnetic field by Schwarzschild black hole. Ann. Inst. H. Poincaré Phys. Théor. 54, 261–320 (1991)

4. A. Bachelot, Scattering of electromagnetic field by de Sitter–Schwarzschild black hole in Non-linear hyperbolic equations and field theory. Pitman Res. Notes Math. Ser. 253, London: Pitman, 1992, pp. 23–35

5. Bachelot A., Motet-Bachelot A.: Les résonances d’un trou noir de Schwarzschild. Ann. Inst. H. Poincaré Phys. Théor. 59, 3–68 (1993)

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