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Gravitational waves via Kerr/CFTAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Christopher Moore. Massive objects orbiting a near-extreme Kerr black hole plunge into the horizon after passing the innermost stable circular orbit, producing a potentially observable signal of gravitational radiation. The near horizon dynamics of such rapidly rotating black holes is governed by a conformal symmetry. In the talk I will show how this symmetry can be exploited to analytically compute the gravitational waves produced by a variety of orbits. I will also discuss an application to gravitational self-force and comment on the holographic interpretation of the process. This talk is part of the DAMTP Friday GR Seminar series. This talk is included in these lists:
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