Abstract

Space-based gravitational wave (GW) detectors will be able to observe signals from sources that are otherwise nearly impossible from current ground-based detection. Consequently, the well established signal detection method, matched filtering, will require a complex template bank, leading to a computational cost that is too expensive in practice. Here, we develop a high-accuracy GW signal detection and extraction method for all space-based GW sources. As a proof of concept, we show that a science-driven and uniform multi-stage self-attention-based deep neural network can identify synthetic signals that are submerged in Gaussian noise. Our method exhibits a detection rate exceeding 99% in identifying signals from various sources, with the signal-to-noise ratio at 50, at a false alarm rate of 1%. while obtaining at least 95% similarity compared with target signals. We further demonstrate the interpretability and strong generalization behavior for several extended scenarios.

Gravitational wave (GW) astronomy has opened a new window of opportunity for our understanding of the Universe, but GW data processing is notoriously complicated due to high noise. Here the authors present a proof-of-concept data analysis scheme based on neural networks for GW signals detection of data from future space-based observatories.

Details

Title
Space-based gravitational wave signal detection and extraction with deep neural network
Author
Zhao, Tianyu 1   VIAFID ORCID Logo  ; Lyu, Ruoxi 2 ; Wang, He 3   VIAFID ORCID Logo  ; Cao, Zhoujian 4   VIAFID ORCID Logo  ; Ren, Zhixiang 5   VIAFID ORCID Logo 

 Beijing Normal University, Department of Astronomy, Beijing, China (GRID:grid.20513.35) (ISNI:0000 0004 1789 9964); Beijing Normal University, Institute for Frontiers in Astronomy and Astrophysics, Beijing, China (GRID:grid.20513.35) (ISNI:0000 0004 1789 9964); Peng Cheng Laboratory, Shenzhen, China (GRID:grid.508161.b) (ISNI:0000 0005 0389 1328) 
 University of Auckland, Department of Statistics, Auckland, New Zealand (GRID:grid.9654.e) (ISNI:0000 0004 0372 3343) 
 University of Chinese Academy of Sciences (UCAS), International Centre for Theoretical Physics Asia-Pacific, Beijing, China (GRID:grid.410726.6) (ISNI:0000 0004 1797 8419); Taiji Laboratory for Gravitational Wave Universe, UCAS, Beijing, China (GRID:grid.410726.6) (ISNI:0000 0004 1797 8419); Chinese Academy of Sciences, CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Beijing, China (GRID:grid.9227.e) (ISNI:0000000119573309) 
 Beijing Normal University, Department of Astronomy, Beijing, China (GRID:grid.20513.35) (ISNI:0000 0004 1789 9964); Beijing Normal University, Institute for Frontiers in Astronomy and Astrophysics, Beijing, China (GRID:grid.20513.35) (ISNI:0000 0004 1789 9964); Hangzhou Institute for Advanced Study, UCAS, School of Fundamental Physics and Mathematical Sciences, Hangzhou, China (GRID:grid.410726.6) (ISNI:0000 0004 1797 8419) 
 Peng Cheng Laboratory, Shenzhen, China (GRID:grid.508161.b) (ISNI:0000 0005 0389 1328) 
Pages
212
Publication year
2023
Publication date
2023
Publisher
Nature Publishing Group
e-ISSN
23993650
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2849187506
Copyright
© The Author(s) 2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.