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Paper

Quadratic quasi-normal mode dependence on linear mode parity

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Leather,  Benjamin
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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2405.10270.pdf
(Preprint), 7MB

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Citation

Bourg, P., Macedo, R. P., Spiers, A., Leather, B., Bonga, B., & Pound, A. (in preparation). Quadratic quasi-normal mode dependence on linear mode parity.


Cite as: https://hdl.handle.net/21.11116/0000-000F-4D8C-E
Abstract
Quasi-normal modes (QNMs) uniquely describe the gravitational-wave ringdown
of post-merger black holes. While the linear QNM regime has been extensively
studied, recent work has highlighted the importance of
second-perturbative-order, quadratic QNMs (QQNMs) arising from the nonlinear
coupling of linear QNMs. Previous attempts to quantify the magnitude of these
QQNMs have shown discrepant results. Using a new hyperboloidal framework, we
resolve the discrepancy by showing that the QQNM/QNM ratio is a function not
only of the black hole parameters but also of the ratio between even- and
odd-parity linear QNMs: the ratio QQNM/QNM depends on what created the ringing
black hole, but only through this ratio of even- to odd-parity linear
perturbations.