Complete parameter inference for GW150914 using deep learning

Stephen Green, J. R. Gair

Machine Learning Science and Technology 2021 article cited by 112

importance 6/10 ai assisted Pulsars and Gravitational Waves Research gravitational-wave astronomy stage: research

Iterative MCMC sampling for gravitational-wave parameter inference is computationally costly as detection rates grow and fast multimessenger alerts are needed.

Growing detector sensitivity increases detections, making rapid inference essential.

A neural-network conditional density estimator (normalizing flows, neural spline flow) was trained to learn non-iterative surrogate models of the Bayesian posterior over the full 15-dimensional binary black hole parameter space.

not stated in source

Evidence supports a demonstrated method applied to GW150914; no quantitative accuracy is stated.

Venue Machine Learning Science and Technology
Published 2021
Work type article
Authors Stephen Green, J. R. Gair
Citations 112 (OpenAlex, at import time)
References 58
Model or method Normalizing flows (neural spline flow)
Organization not stated in source
Primary source https://doi.org/10.1088/2632-2153/abfaed
Open access gold
Keywords gravitational waves, GW150914, normalizing flows, deep learning, parameter inference, Bayesian posterior
6 / 10

significant — thousands to millions affected

Abstract states detection rates grow with detector sensitivity and fast multimessenger alerts are needed; supports a major physics field, but no quantified scale given.

Basis: stated. The source itself states the scale. Stated scale: not stated in source. Method and limits.

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