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  • Letter

Explaining nonlinearities in black hole ringdowns from symmetries

Alex Kehagias1,2,*, Davide Perrone3,†, Antonio Riotto3,4,‡, and Francesco Riva3,§

  • 1Physics Department, National Technical University of Athens, 15780 Athens, Greece
  • 2CERN, Theoretical Physics Department, CH-1211 Geneva, Switzerland
  • 3Département de Physique Théorique, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Geneva, Switzerland
  • 4Gravitational Wave Science Center (GWSC), Université de Genève, 24 quai Ernest Ansermet, CH-1211 Geneva, Switzerland

  • *kehagias@central.ntua.gr
  • †davide.perrone@unige.ch
  • ‡antonio.riotto@unige.ch
  • §francesco.riva@unige.ch

Phys. Rev. D 108, L021501 – Published 10 July, 2023

DOI: https://doi.org/10.1103/PhysRevD.108.L021501

Abstract

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 behavior is explained, both on the qualitative and quantitative level, by near-horizon symmetries of the Kerr black hole within the Kerr/CFT correspondence.

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