The development of thermodynamically consistent and physics-informed equation-of-state model through machine learning

J. Hinz, Dayou Yu, Deep Shankar Pandey, Hitesh Sapkota, Qi Yu, D. Mihaylov, V. V. Karasiev, S. Hu
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Abstract

Ab initio molecular dynamics (AIMD) simulations have become an important tool used in the construction of equations of state (EOS) tables for warm dense matter. Due to computational costs, only a limited number of system state conditions can be simulated, and the remaining EOS surface must be interpolated for use in radiation-hydrodynamic simulations of experiments. In this work, we develop a thermodynamically consistent EOS model that utilizes a physics-informed machine learning approach to implicitly learn the underlying Helmholtz free-energy from AIMD generated energies and pressures. The model, referred to as PIML-EOS, was trained and tested on warm dense polystyrene producing a fit within a 1% relative error for both energy and pressure and is shown to satisfy both the Maxwell and Gibbs–Duhem relations. In addition, we provide a path toward obtaining thermodynamic quantities, such as the total entropy and chemical potential (containing both ionic and electronic contributions), which are not available from current AIMD simulations.
通过机器学习开发热力学一致和物理信息的状态方程模型
原子分子动力学(AIMD)模拟已成为构建热致密物质状态方程(EOS)表的重要工具。由于计算成本的原因,只能模拟有限数量的系统状态条件,其余的 EOS 表必须内插到辐射流体力学模拟实验中使用。在这项工作中,我们开发了一种热力学一致的 EOS 模型,该模型利用物理信息机器学习方法,从 AIMD 生成的能量和压力中隐含地学习底层赫尔姆霍兹自由能。该模型被称为 PIML-EOS,在暖致密聚苯乙烯上进行了训练和测试,能量和压力的拟合相对误差均在 1%以内,并证明它同时满足麦克斯韦和吉布斯-杜恒关系。此外,我们还提供了一条获得热力学量的途径,如总熵和化学势(包含离子和电子贡献),这些都是目前的 AIMD 模拟无法获得的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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