Pith. sign in

REVIEW 4 cited by

Enhancing Gravitational-Wave Science with Machine Learning

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2005.03745 v2 pith:5GLWZMVD submitted 2020-05-07 astro-ph.HE gr-qc

classification astro-ph.HEgr-qc
keywords gravitational-wavelearningmachinetechniquesadvancedapplicationsdetectorscience
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Machine learning has emerged as a popular and powerful approach for solving problems in astrophysics. We review applications of machine learning techniques for the analysis of ground-based gravitational-wave detector data. Examples include techniques for improving the sensitivity of Advanced LIGO and Advanced Virgo gravitational-wave searches, methods for fast measurements of the astrophysical parameters of gravitational-wave sources, and algorithms for reduction and characterization of non-astrophysical detector noise. These applications demonstrate how machine learning techniques may be harnessed to enhance the science that is possible with current and future gravitational-wave detectors.

Discussion (0). Sign in to comment.

Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Predicting intermediate-mass black hole formation in star clusters with machine learning

    astro-ph.GA 2026-05 unverdicted novelty 7.0 of 10

    Machine learning regressors trained on Rapster simulations forecast that globular clusters rarely host black holes above 100 solar masses while a few nuclear star clusters may exceed this threshold.

  2. Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection

    gr-qc 2026-05 unverdicted novelty 7.0 of 10

    A contrastive self-supervised convolutional autoencoder detects core-collapse supernova gravitational waves with performance comparable to supervised CNNs, better generalization to unseen waveforms, and ~120 kpc sensi...

  3. Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    A CNN framework using response functions from gravitational wave mismatches classifies signals as GR or beyond-GR with 33 times better sensitivity than raw waveforms and detects massive gravity deviations at graviton ...

  4. Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data

    gr-qc 2025-05 unverdicted novelty 5.0 of 10

    GP15 maps BBH spectrograms to parameter posteriors via residual networks and normalizing flows, producing results consistent with LVK analyses on GWTC-2.1 and GWTC-3 events while running in seconds.

Pith tools