Neural likelihood estimators for flexible Gravitational wave data analysis

ABSTRACT In this paper, we develop a Neural Likelihood Estimator and apply it to analyse real gravitational-wave (GW) data for the first time. We assess the usability of neural likelihood for GW parameter estimation and report the parameter space where neural likelihood performs as a robust estimator to output posterior probability distributions using modest computational resources. In addition, we demonstrate that the trained Neural likelihood can also be used in further analysis, enabling us to obtain the evidence corresponding to a hypothesis, making our method a complete tool for parameter estimation. Particularly, our method requires around 100 times fewer likelihood evaluations than standard Bayesian algorithms to infer properties of a GW signal from a binary black hole system as observed by current generation ground-based detectors. The fairly simple neural network architecture chosen makes for cheap training, which allows our method to be used on-the-fly without the need for special hardware and ensures our method is flexible to use any waveform model, noise model, or prior. We show results from simulations as well as results from GW150914 as proof of the effectiveness of our algorithm.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2026-01-22
DOI
https://doi.org/10.1093/mnras/staf2145
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00

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article

Neural likelihood estimators for flexible Gravitational wave data analysis

Luca Negri, Anuradha Samajdar
Monthly Notices of the Royal Astronomical Society
Pulsars and Gravitational Waves Research
article

Neural likelihood estimators for flexible Gravitational wave data analysis

Luca Negri, Anuradha Samajdar
article en

Abstract

ABSTRACT In this paper, we develop a Neural Likelihood Estimator and apply it to analyse real gravitational-wave (GW) data for the first time. We assess the usability of neural likelihood for GW parameter estimation and report the parameter space where neural likelihood performs as a robust estimator to output posterior probability distributions using modest computational resources. In addition, we demonstrate that the trained Neural likelihood can also be used in further analysis, enabling us to obtain the evidence corresponding to a hypothesis, making our method a complete tool for parameter estimation. Particularly, our method requires around 100 times fewer likelihood evaluations than standard Bayesian algorithms to infer properties of a GW signal from a binary black hole system as observed by current generation ground-based detectors. The fairly simple neural network architecture chosen makes for cheap training, which allows our method to be used on-the-fly without the need for special hardware and ensures our method is flexible to use any waveform model, noise model, or prior. We show results from simulations as well as results from GW150914 as proof of the effectiveness of our algorithm.

Monthly Notices of the Royal Astronomical SocietyVol. 546(2)
Utrecht University (NL), National Institute for Subatomic Physics (NL)
National Science Foundation, Science and Technology Facilities Council
Openalex Percentile: Top 76%
Pulsars and Gravitational Waves Research
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