Dilated convolutional neural network for detecting extreme-mass-ratio inspirals (2308.16422v3)
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 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 1-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.
- A. Sesana, Phys. Rev. Lett. 116, 231102 (2016).
- P. Amaro-Seoane, H. Audley, S. Babak, J. Baker, E. Barausse, P. Bender, E. Berti, et al., “Laser Interferometer Space Antenna,” (2017), 1702.00786 .
- W.-R. Hu and Y.-L. Wu, Natl. Sci. Rev. 4, 685 (2017).
- P. Auclair, D. Bacon, T. Baker, T. Barreiro, N. Bartolo, et al., “Cosmology with the Laser Interferometer Space Antenna,” (2022), arxXiv:2204.05434 .
- LISA Science Study Team, LISA Science Requirements Document, Tech. Rep. ESA-L3-EST-SCI-RS-001 (\aclESA, 2018).
- W.-B. Han and X. Chen, Mon. Not. R. Astron. Soc.: Lett 485, L29 (2019).
- J. Gair and L. Wen, Class. Quantum Gravity 22, S1359 (2005).
- L. Wen and J. R. Gair, Class. Quantum Gravity 22, S445 (2005).
- J. Gair and G. Jones, Class. Quantum Gravity 24, 1145 (2007).
- D. George and E. A. Huerta, Phys. Rev. D 97, 044039 (2018).
- P. G. Krastev, Phys. Lett. B 803, 135330 (2020).
- V. Skliris, M. R. K. Norman, and P. J. Sutton, “Real-Time Detection of Unmodelled Gravitational-Wave Transients Using Convolutional Neural Networks,” (2022), arXiv:2009.14611 .
- A. Ravichandran, A. Vijaykumar, S. J. Kapadia, and P. Kumar, “Rapid identification and classification of eccentric gravitational wave inspirals with machine learning,” (2023), arXiv:2302.00666 .
- M. Razzano and E. Cuoco, Class. Quantum Gravity 35, 095016 (2018).
- L. Barack and C. Cutler, Phys. Rev. D 69, 082005 (2004).
- A. J. K. Chua and J. R. Gair, Class. Quantum Gravity 32, 232002 (2015).
- S. Bai, J. Z. Kolter, and V. Koltun, “An empirical evaluation of generic convolutional and recurrent networks for sequence modeling,” (2018), arXiv:1803.01271 .
- T. Salimans and D. P. Kingma, in Advances in Neural Information Processing Systems, Vol. 29 (Curran Associates, Inc., 2016).
- C. M. Bishop, Pattern Recognition and Machine Learning, softcover reprint of the original 1st edition 2006 (corrected at 8th printing 2009) ed., Information Science and Statistics (Springer New York, New York, NY, 2016).