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

被引:3
作者
Zhao, Tianyu [1 ,2 ,3 ]
Zhou, Yue [2 ]
Shi, Ruijun [1 ,3 ]
Cao, Zhoujian [1 ,3 ,4 ]
Ren, Zhixiang [1 ,2 ]
机构
[1] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
[2] Peng Cheng Lab, Shenzhen 518055, Peoples R China
[3] Beijing Normal Univ, Inst Frontiers Astron & Astrophys, Beijing 102206, Peoples R China
[4] UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China
关键词
TESTING GENERAL-RELATIVITY; SPACE; PHYSICS;
D O I
10.1103/PhysRevD.109.084054
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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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页数:11
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