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University of Cambridge > Talks.cam > DAMTP Friday GR Seminar > Computing the second order curvature perturbations of Kerr black holes
Computing the second order curvature perturbations of Kerr black holesAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Justin Ripley. I will describe a formalism to compute the second order gravitational (vacuum) perturbations of Kerr black holes, a numerical code that implements that formalism, and example output from the code. To motivate this work, I will discuss several applications where going beyond linear perturbation theory may be necessary, including modeling the “ringdown” of (near extremal) Kerr black holes, modeling “black hole turbulence”, and the self-force problem. I will discuss what our current results have to say on those issues, and directions for future work. This talk is part of the DAMTP Friday GR Seminar series. This talk is included in these lists:
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