Dilated convolutional neural network for detecting extreme-mass-ratio inspirals

Tianyu Zhao, Yue Zhou, Ruijun Shi, Zhoujian Cao, and Zhixiang Ren
Phys. Rev. D 109, 084054 – Published 23 April 2024

Abstract

The detection of extreme-mass-ratio inspirals (EMRIs) is intricate due to their complex waveforms, extended duration, and low signal-to-noise ratio (SNR), making them more challenging to be identified compared to compact binary coalescences. While matched filtering-based techniques are known for their computational demands, existing deep learning-based methods primarily handle time-domain data and are often constrained by data duration and SNR. In addition, most existing work ignores time delay interferometry (TDI) and applies the long-wavelength approximation in detector response calculations, thus limiting their ability to handle laser frequency noise. In this study, we introduce dilated convolutional neural network for detecting extreme-mass-ratio inspirals (DECODE), an end-to-end model focusing on EMRI signal detection by sequence modeling in the frequency domain. Centered around a dilated causal convolutional neural network, trained on synthetic data considering TDI-1.5 detector response, DECODE can efficiently process a year’s worth of multichannel TDI data with an SNR of around 50. We evaluate our model on one-year data with accumulated SNR ranging from 50 to 120 and achieve a true positive rate of 96.3% at a false positive rate of 1%, keeping an inference time of less than 0.01 seconds. With the visualization of three showcased EMRI signals for interpretability and generalization, DECODE exhibits strong potential for future space-based gravitational wave data analyses.

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  • Received 1 September 2023
  • Accepted 28 March 2024

DOI:https://doi.org/10.1103/PhysRevD.109.084054

© 2024 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & AstrophysicsInterdisciplinary Physics

Authors & Affiliations

Tianyu Zhao1,2,3, Yue Zhou2, Ruijun Shi1,3, Zhoujian Cao1,3,4,*, and Zhixiang Ren2,†

  • 1Department of Astronomy, Beijing Normal University, Beijing 100875, China
  • 2Peng Cheng Laboratory, Shenzhen, 518055, China
  • 3Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, China
  • 4School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, UCAS, Hangzhou 310024, China

  • *Corresponding author: zjcao@bnu.edu.cn
  • Corresponding author: renzhx@pcl.ac.cn

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Issue

Vol. 109, Iss. 8 — 15 April 2024

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