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Explaining Nonlinearities in Black Hole Ringdowns from Symmetries

by Antonio Walter Riotto (Universite de Geneve (CH))

Europe/Zurich
4/2-011 - TH common room (CERN)

4/2-011 - TH common room

CERN

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Description

It has been recently pointed out that nonlinear effects are necessary to model the ringdown stage of the gravitational waveform produced by the merger of two black holes giving rise to a remnant Kerr black hole. We show that this nonlinear behaviour is explained, both on the qualitative and quantitative level, by near-horizon symmetries of the Kerr black hole within the Kerr/CFT correspondence.