Normalizing flows for density estimation in multi-detector gravitational-wave searches
Sam Insley, Michael J. Williams, Rahul Dhurkunde, Ian Harry

TL;DR
This paper introduces normalizing flows as an efficient density estimation method to improve gravitational-wave event significance assessment, reducing storage needs and increasing sensitivity in multi-detector searches.
Contribution
It demonstrates that normalizing flows can replace histogram-based estimators in PyCBC, enabling scalable analysis with minimal sensitivity loss and improved detection capabilities.
Findings
Normalizing flows reduce storage by over 1000 times.
Less than 0.05% drop in signal recovery at fixed false-alarm rate.
Up to 6.55% increase in recovered signals for certain detector combinations.
Abstract
Identifying compact binary coalescences buried within the non-Gaussian and non-stationary data taken by gravitational-wave interferometers requires sophisticated search pipelines, such as the PyCBC analysis. A critical task for these pipelines is determining the statistical significance of candidate events by comparing a "ranking statistic" against a large background set. Currently, PyCBC's ranking statistic incorporates the joint probability of the relative arrival times, phase delays and amplitude ratios of the signals seen in different detectors. These parameters are tightly constrained for physical signals but are more broadly distributed for noise. PyCBC currently relies on precomputed binned histogram-based density estimators using Monte-Carlo simulations to obtain these probabilities. However, the storage requirements for these histograms scale prohibitively with the size of the…
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