基于物理信息驱动傅里叶神经算子的Vlasov方程求解方法

Method for solving Vlasov equation based on physics-informed Fourier neural operator

  • 摘要: Vlasov方程是研究等离子体物理的重要方程,在高温、完全电离且忽略库伦碰撞的情况下,其数值求解方法主要有欧拉类方法和拉格朗日类方法。考虑传统数值求解方法在高精度网格条件下计算资源快速增长、维度灾难等问题,采用了基于物理信息驱动的傅里叶神经算子(PFNO)对Vlasov方程进行求解。该方法将傅里叶神经算子高维函数映射能力与Vlasov方程物理约束结合,构建了数据-物理信息驱动的深度学习框架,可提升模型在稀疏数据条件下的泛化性能,同时具有网格无关性特征。数值实验表明,该方法在保证求解精度的同时,相比传统有限元法和谱方法计算效率提升1~2个数量级,且能并行处理大批量数据。该研究为高维Vlasov动力学方程的求解提供了新思路,在惯性约束聚变、空间等离子体模拟等领域具有一定应用潜力。

     

    Abstract:
    Background
    The Vlasov equation is a cornerstone in plasma physics, governing the evolution of distribution functions in high-temperature, collisionless plasmas. Conventional numerical methods, including Eulerian and Lagrangian approaches, often encounter severe computational challenges due to the rapid increase in cost with fine grid resolutions and the curse of dimensionality. These limitations restrict their effectiveness in large-scale kinetic plasma simulations needed in fusion research and space plasma studies.
    Purpose
    This work aims to develop an efficient and scalable computational framework for solving the Vlasov equation that mitigates the drawbacks of traditional methods. The study particularly addresses the need for maintaining accuracy and physical consistency while significantly reducing computational costs in high-dimensional simulations. An approach based on the physics-informed Fourier neural operator (PFNO) is introduced.
    Methods
    The method integrates the high-dimensional function mapping ability of the fourier neural operator with the physical constraints of the Vlasov equation. A physics-informed loss function is constructed to enforce mass, momentum, and energy conservation laws. The framework was evaluated through benchmark tests against finite element and spectral solvers, and its parallel performance was assessed on large-scale computing platforms.
    Results
    The PFNO approach demonstrates accuracy comparable to conventional solvers while achieving computational efficiency improvements of one to two orders of magnitude. The method shows strong generalization under sparse-data conditions, exhibits grid independence, and scales effectively in parallel computing environments, enabling efficient treatment of high-dimensional plasma dynamics. The study presents a novel paradigm for solving high-dimensional Vlasov equations by combining deep learning operators with physical principles.
    Conclusions
    The PFNO framework enhances efficiency without sacrificing physical accuracy, making it a promising tool for applications in inertial confinement fusion, astrophysical plasma modeling, and space plasma simulations. Future research directions include extension to multi-species and relativistic plasma systems.

     

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