Gravitational wave signal extraction against non-stationary instrumental noises with deep neural network

IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Physics Letters B Pub Date : 2024-09-12 DOI:10.1016/j.physletb.2024.139016
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Abstract

Sapce-borne gravitational wave antennas, such as LISA and LISA-like mission (Taiji and Tianqin), will offer novel perspectives for exploring our Universe while introduce new challenges, especially in data analysis. Aside from the known challenges like high parameter space dimension, superposition of large number of signals etc., gravitational wave detections in space would be more seriously affected by anomalies or non-stationarities in the science measurements. Considering the three types of foreseeable non-stationarities including data gaps, transients (glitches), and time-varying noise auto-correlations, which may come from routine maintenance or unexpected disturbances during science operations, we developed a deep learning model for accurate signal extractions confronted with such anomalous scenarios. Our model exhibits the same performance as the current state-of-the-art models do for the ideal and anomaly free scenario, while shows remarkable adaptability in extractions of coalescing massive black hole binary signal against all three types of non-stationarities and even their mixtures. This also provide new explorations into the robustness studies of deep learning models for data processing in space-borne gravitational wave missions.

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利用深度神经网络提取引力波信号,对抗非稳态仪器噪声
星载引力波天线,如 LISA 和类 LISA 任务(太极和天琴),将为探索我们的宇宙提供新的视角,同时也带来了新的挑战,特别是在数据分析方面。除了高参数空间维度、大量信号叠加等已知挑战外,科学测量中的异常或非稳态现象将对空间引力波探测产生更严重的影响。考虑到三类可预见的非稳态,包括数据间隙、瞬态(小故障)和时变噪声自相关(可能来自日常维护或科学运作过程中的意外干扰),我们开发了一种深度学习模型,用于面对此类异常情况时精确提取信号。我们的模型在理想和无异常场景下表现出与当前最先进模型相同的性能,同时在提取凝聚大质量黑洞双星信号时,针对所有三种类型的非稳态,甚至是它们的混合物,都表现出显著的适应性。这也为天基引力波任务中数据处理深度学习模型的鲁棒性研究提供了新的探索。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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