Exploring gravitational-wave detection and parameter inference using deep learning methods

João D Álvares, José A. Font, Felipe F Freitas, Osvaldo G Freitas, António P Morais, Solange Nunes, Antonio Onofre, Alejandro Torres-Forné

Classical and Quantum Gravity 2021 article cited by 21

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

Detecting gravitational-wave signals from binary black hole mergers in noisy detector data and inferring their parameters.

Faster gravitational-wave detection could enable timely follow-up observations of cosmic events.

Deep learning networks trained on BBH merger waveforms injected into real LIGO/Virgo O2 data performed detection, and a regression network performed parameter inference.

High detection accuracy for signals up to 2000 Mpc; combining three detectors into one RGB image improved single-detector performance by up to 70%.

Demonstrates deep learning as a viable method for gravitational-wave detection and inference on real detector data.

Venue Classical and Quantum Gravity
Published 2021
Work type article
Authors João D Álvares, José A. Font, Felipe F Freitas, Osvaldo G Freitas, António P Morais, Solange Nunes, Antonio Onofre, Alejandro Torres-Forné
Citations 21 (OpenAlex, at import time)
References 59
Model or method not stated in source
Organization not stated in source
Primary source https://doi.org/10.1088/1361-6382/ac0455
Open access bronze
Keywords gravitational waves, deep learning, black hole mergers, LIGO, parameter inference
6 / 10

significant — thousands to millions affected

Gravitational-wave detection supports a foundational scientific field (multi-messenger astronomy); abstract shows viability on real LIGO/Virgo data but states no scale of impact.

Basis: inferred. Judged from the source text, which gives no explicit scale. Stated scale: not stated in source. Method and limits.

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