📝 SummarXiv

Abstract

We present a comprehensive investigation of the F-statistic method for parameter estimation of gravitational wave (GW) signals from binary black hole mergers. By analytically maximizing the likelihood over the luminosity distance and polarization angle, this approach reduces the dimensionality of the parameter space to enhance computational efficiency. We also introduce a novel formulation for calculating the Bayes factor for the F-statistic, enabling a quantitative assessment of its performance against standard full frequency-domain (FFD) Bayesian inference. Using the benchmark event GW150914, we demonstrate that the F-statistic method is not only approximately $70\%$ faster than FFD but is also statistically stable across different sampler configurations, with a log-Bayes factor between runs smaller than $0.1$. Furthermore, the F-statistic exhibits superior stability against changes in sampler configuration, yielding consistently lower Jensen-Shannon divergence values between analysis runs. While the F-statistic produces slightly broader constraints on some parameters, we argue this represents a more honest uncertainty quantification, particularly in high-dimensional parameter spaces with complex posterior structures. These results highlight the significant advantages of the F-statistic method for GW data analysis, positioning it as a powerful tool for the era of high-rate detections with future observatories.