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Detecting gravitational waves from extreme mass ratio inspirals using convolutional neural networks

Xue-Ting Zhang, Chris Messenger, Natalia Korsakova, Man Leong Chan, Yi-Ming Hu, and Jian-dong Zhang
Phys. Rev. D 105, 123027 – Published 24 June 2022

Abstract

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 toward different waveform models. Our study reveals the potential applicability of machine learning technology like CNNs toward more realistic EMRI data analysis.

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  • Received 14 February 2022
  • Accepted 9 June 2022

DOI:https://doi.org/10.1103/PhysRevD.105.123027

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Xue-Ting Zhang1, Chris Messenger2, Natalia Korsakova3, Man Leong Chan4, Yi-Ming Hu1,*, and Jian-dong Zhang1

  • 1MOE Key Laboratory of TianQin Mission, TianQin Research Center for Gravitational Physics and School of Physics and Astronomy, Frontiers Science Center for TianQin, Gravitational Wave Research Center of CNSA, Sun Yat-sen University (Zhuhai Campus), Zhuhai 519082, China
  • 2SUPA, School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
  • 3ARTEMIS, Observatoire de la Côte d’Azur, Boulevard de l’Observatoire, 06304 Nice, France
  • 4Department of Applied Physics, Fukuoka University, Nanakuma 8-19-1, Fukuoka 814-0180, Japan

  • *huyiming@mail.sysu.edu.cn

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Issue

Vol. 105, Iss. 12 — 15 June 2022

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Images

  • Figure 1
    Figure 1

    An example EMRI signals compared with the sensitivity curve of TianQin. A total length of 3 months observation time is assumed.

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  • Figure 2
    Figure 2

    An example of whitened data in channel I in comparison with signal hI alone. For this event, the SNR is set to be 50. We draw the reader’s attention to the difference in scale for the noise and the signal.

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  • Figure 3
    Figure 3

    The ROC curve of the signals from testing groups 1–3 is shown with the blue, purple, and red lines, respectively. The blue line indicates the expected effectiveness for group 1, the parameters have identical distribution to the training data; for group 2, the distribution is drawn from an astrophysical model; for group 3, the distribution is the same as group 1 and the training data, but switched to the AAK waveform model. The 1σ confidence intervals are indicated by the shaded regions.

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  • Figure 4
    Figure 4

    The comparison of the CNN sensitivity over EMRIs with different parameters. The vertical axis is the TAP, while the horizontal axis is the single varying parameter. The 1σ confidence intervals are indicated by the shaded regions. (a), (b), (c), and (d) correspond to testing data from group 4, 5, 6, and 7, respectively.

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