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arXiv 2607.06002gr-qc
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用物理信息神经网络求解哈密顿约束方程

Solving Hamiltonian Constraint Equation with Physics-Informed Neural Networks

Hangzhou Institute for Advanced Study, UCAS(杭州高等研究院,中国科学院大学);Department of Artificial Intelligence, School of Engineering, Westlake University(西湖大学工学院人工智能系);School of Physical Sciences, University of Chinese Academy of Sciences(中国科学院大学物理科学学院);International Centre for Theoretical Physics Asia-Pacific, University of Chinese Academy of Sciences(中国科学院大学亚太理论物理中心);Department of Astronomy, Westlake University(西湖大学天文学系);Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University(北京师范大学天文与前沿科学研究院);School of Physics and Astronomy, Beijing Normal University(北京师范大学物理与天文学院);National Astronomical Observatories, Chinese Academy of Sciences(中国科学院国家天文台);Fudan Center for Mathematics and Interdisciplinary Study, Fudan University(复旦大学数学交叉研究中心)

Yu-Chen Zhou, Hao Ma, Zhoujian Cao, Tailin Wu, Hong-Bo Jin, Xuefeng Feng, Shuanglin Huang, Zhi-Chao Zhao, Yue-Liang Wu

AI总结:

研究数值相对论中双黑洞初始数据的哈密顿约束方程求解问题,提出物理信息神经网络(PINN)方法并引入新技术,成功求解该方程,验证了方法高精度和鲁棒性,展现构建基于PINN初始数据解的潜力。

摘要:

数值相对论在引力波天文学的源建模中起着重要作用,传统数值方法已成熟,但用于偏微分方程的神经网络方法在数值相对论中研究不足。本文提出一种物理信息神经网络(PINN)方法来求解数值相对论中双黑洞(BBH)初始数据的哈密顿约束方程,该方程是高度非线性椭圆偏微分方程,为此引入新技术。结果表明PINN结合这些技术能成功求解一般BBH系统的哈密顿约束方程,验证了方法的高精度和鲁棒性,揭示了构建基于PINN的初始数据解的巨大潜力。

英文摘要:

Numerical relativity (NR), solving Einstein equation numerically, plays an important role in source modelling for gravitational wave astronomy. Traditional methods for NR including finite difference method, spectral method and finite element method have been well developed. But newly developed neural network methods for partial differential equations (PDE) have not been well studied yet for NR. We present a Physics-Informed Neural Network (PINN) method to solve the Hamiltonian constraint equation for binary black hole (BBH) initial data in NR. This equation is a highly non-linear elliptic PDE, posing significant challenges for conventional PINN approaches. To overcome these difficulties, we introduce a set of new techniques. We show that our PINN together with these techniques can successfully solve the Hamiltonian constraint equation for generic BBH systems. Validation against the traditional results demonstrates the high accuracy and robustness of our method, revealing the immense potential of constructing a PINN-based initial data solution to all BBH systems for NR.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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