pith. sign in

A practical Bayesian method for gravitational-wave ringdown analysis with multiple modes

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

Gravitational-wave (GW) ringdown signals from black holes (BHs) encode crucial information about the gravitational dynamics in the strong-field regime, which offers unique insights into BH properties. In the future, the improving sensitivity of GW detectors is to enable the extraction of multiple quasi-normal modes (QNMs) from ringdown signals. However, incorporating multiple modes drastically enlarges the parameter space, posing computational challenges to data analysis. Inspired by the $F$-statistic method in the continuous GW searches, we develope an algorithm, dubbed as FIREFLY, for accelerating the ringdown signal analysis. FIREFLY analytically marginalizes the amplitude and phase parameters of QNMs to reduce the computational cost and speed up the full-parameter inference from hours to minutes, while achieving consistent posterior and evidence. The acceleration becomes more significant when more QNMs are considered. Rigorously based on the principle of Bayesian inference and importance sampling, our method is statistically interpretable, flexible in prior choice, and compatible with various advanced sampling techniques, providing a new perspective for accelerating future GW data analysis.

citation-role summary

background 1

citation-polarity summary

years

2026 2 2025 1

roles

background 1

polarities

background 1

clear filters

representative citing papers

citing papers explorer

Showing 2 of 2 citing papers after filters.

  • Cracking Gravitational Wave Multiple Ringdown Modes in Space gr-qc · 2026-04-22 · unverdicted · none · ref 11 · internal anchor

    FIREFLY algorithm enables 200-fold faster multi-mode ringdown analysis for space-borne gravitational wave detectors while remaining compatible with time-delay interferometry.

  • FluxMC: Rapid and High-Fidelity Inference for Space-Based Gravitational-Wave Observations astro-ph.IM · 2026-04-03 · unverdicted · none · ref 7 · internal anchor

    FluxMC integrates flow matching with parallel tempering MCMC to converge in under five hours on high-fidelity IMRPhenomHM waveforms for massive black hole binaries, where standard methods fail after hundreds of hours and produce two to three orders of magnitude higher distributional error.