Quasinormal Mode Content of Binary Black Hole Ringdowns
Abstract
We present a fully Bayesian, data-driven framework for identifying quasinormal modes in high-accuracy Cauchy characteristic evolution gravitational waveforms. Applying this to a public catalog, we identify quasinormal mode overtones, retrograde modes, and nonlinear modes up to cubic order in the ringdown. Multiple high-order overtones are found near the merger, confirming their physical significance for modeling the ringdown. The ringdown mode content is tabulated across a wide range of start times for all available simulations, providing a systematic reference for theoretical and observational studies. We also search for late-time power-law tails, which are, as expected, absent from the Cauchy characteristic evolution waveforms.
Fields of Study & Subjects
Black Holes and Theoretical Physics
Pulsars and Gravitational Waves Research
Astrophysical Phenomena and Observations
Publication details
- Journal / source
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Volume
- 136
- Issue
- 19
- Pages
- 191403–191403
- Publication date
- 26 March 2026
- Language
- EN