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Detecting Gravitational-waves from Extreme Mass Ratio Inspirals using Convolutional Neural Networks

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arxiv 2202.07158 v1 pith:AUDWYNRW submitted 2022-02-15 astro-ph.HE gr-qc

classification astro-ph.HEgr-qc
keywords emriratioanalysiscnnsconvolutionaldataextremeinspirals
verification ladder T0 review T1 audit T2 compute T3 formal
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Extreme mass ratio inspirals (EMRIs) are among the most interesting gravitational wave (GW) sources for space-borne GW detectors. However, successful GW data analysis remains challenging due to many issues, ranging from the difficulty of modeling accurate waveforms, to the impractically large template bank required by the traditional matched filtering search method. In this work, we introduce a proof-of-principle approach for EMRI detection based on convolutional neural networks (CNNs). We demonstrate the performance with simulated EMRI signals buried in Gaussian noise. We show that over a wide range of physical parameters, the network is effective for EMRI systems with a signal-to-noise ratio larger than 50, and the performance is most strongly related to the signal-to-noise ratio. The method also shows good generalization ability towards different waveform models. Our study reveals the potential applicability of machine learning technology like CNNs towards more realistic EMRI data analysis.

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Cited by 3 Pith papers

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

  1. Searching for extreme mass ratio inspirals in LISA: from identification to parameter estimation

    gr-qc 2025-05 conditional novelty 6.0 of 10

    A staged pipeline using a new time-frequency match statistic recovers and estimates parameters of two injected EMRI signals in simulated LISA data, though with a hyperparameter tuned on those injections.

  2. Sequential simulation-based inference for extreme mass ratio inspirals

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Sequential simulation-based inference with truncated marginal neural ratio estimation shrinks the 11-parameter search volume for simulated non-spinning extreme-mass-ratio inspirals by factors of 1e6 to 1e7 and recover...

  3. Searching for stellar-origin binary black holes in LISA Data Challenge 1b: Yorsh

    gr-qc 2024-12 conditional novelty 5.0 of 10

    An existing semi-coherent hierarchical search recovers the five loudest injected stellar-origin binary black holes in LISA Data Challenge 1b Yorsh, with SNR as low as 12.94.

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