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Showing 1 to 3 of 3 for “"Kerr de Sitter"”.

  1. Decay for quasilinear wave equations on cosmological black hole backgrounds

    This thesis studies the decay and stability of linear and quasilinear wave equations of Schwarzschild--de~Sitter $(M,\Lambda)$ and Kerr de Sitter $(a,M,\Lambda)$ black hole backgrounds, where $a,M,\Lambda$ are respectively the rotation parameter of the black hole, the mass of the black hole and the …

    cambridge Repository record for Decay for quasilinear wave equations on cosmological black hole backgrounds (opens in a new tab)

  2. Wave Equations on Curved Spacetimes

    … where there are stably trapped null geodesics that have zero energy relative to an observer at infinity. We give a heuristic argument as to why this may lead to a non-linear instability, which can be seen at the linear level by studying the wave equation. We calculate the quasinormal …

    cambridge Repository record for Wave Equations on Curved Spacetimes (opens in a new tab)

  3. Quasinormal Modes of Nearly Extremal Black Holes

    Quasinormal modes are the gravitational wave analogue to the overtones heard after striking a bell; like many physical systems, black holes emit radiation as a response to perturbations. After a dynamical event, for example a black hole merger, the system is expected to relax to a stationary black …

    cambridge Repository record for Quasinormal Modes of Nearly Extremal Black Holes (opens in a new tab)