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Nonlinear effects in black hole ringdown

Published 15 Aug 2022 in gr-qc, astro-ph.HE, and hep-th | (2208.07374v3)

Abstract: We report evidence for nonlinear modes in the ringdown stage of the gravitational waveform produced by the merger of two comparable-mass black holes. We consider both the coalescence of black hole binaries in quasicircular orbits and high-energy, head-on black hole collisions. The presence of nonlinear modes in the numerical simulations confirms that general-relativistic nonlinearities are important and must be considered in gravitational-wave data analysis.

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