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Machine Learning Interatomic Potentials for Million-Atom Simulations of Multicomponent Alloys

Fei Shuang, Penghua Ying, Kai Liu, Zixiong Wei, Fengxian Liu, Zheyong Fan, Minqiang Jiang, Poulumi Dey

Abstract

Machine learning interatomic potentials (MLIPs) with broad chemical flexibility are important for atomistic simulations of compositionally complex materials such as high-entropy alloys. Here, we study two state-of-the-art MLIP frameworks, the neuroevolution potential (NEP) and the graph atomic cluster expansion (GRACE), for 16 elemental metals and multicomponent alloys. GRACE potential with Finnis-Sinclair type shows substantially higher training efficiency and consistently, though only slightly, better accuracy for mechanical properties, thermal stability, and chemical extrapolation. In contrast, NEP achieves an approximately 60-fold higher inference speed, making it attractive for million-atom molecular dynamics simulations. We further examine uncertainty quantification strategies and find that ensemble-based uncertainty correlates robustly with model error, whereas D-optimality is less reliable for the systems considered here. Large-scale nonequilibrium molecular dynamics simulations of shock propagation further show that NEP, combined with ensemble-based uncertainty quantification, enables efficient and reliable simulations under extreme dynamic conditions.

Machine Learning Interatomic Potentials for Million-Atom Simulations of Multicomponent Alloys

Abstract

Machine learning interatomic potentials (MLIPs) with broad chemical flexibility are important for atomistic simulations of compositionally complex materials such as high-entropy alloys. Here, we study two state-of-the-art MLIP frameworks, the neuroevolution potential (NEP) and the graph atomic cluster expansion (GRACE), for 16 elemental metals and multicomponent alloys. GRACE potential with Finnis-Sinclair type shows substantially higher training efficiency and consistently, though only slightly, better accuracy for mechanical properties, thermal stability, and chemical extrapolation. In contrast, NEP achieves an approximately 60-fold higher inference speed, making it attractive for million-atom molecular dynamics simulations. We further examine uncertainty quantification strategies and find that ensemble-based uncertainty correlates robustly with model error, whereas D-optimality is less reliable for the systems considered here. Large-scale nonequilibrium molecular dynamics simulations of shock propagation further show that NEP, combined with ensemble-based uncertainty quantification, enables efficient and reliable simulations under extreme dynamic conditions.

Paper Structure

This paper contains 20 sections, 12 equations, 10 figures, 2 tables.

Figures (10)

  • Figure 1: Benchmarking the accuracy and efficiency of UNEP-v1 and GRACE-FS-M potentials. Error distributions for (a) energy, (b) forces, and (c) virial stress are compared alongside (d) the computational cost (wall time) required for training.
  • Figure 2: Uncertainty quantification for UNEP-v1 and GRACE-FS-M potentials. (a, b) Uncertainty estimates for UNEP-v1 using ensemble learning at the atomic and structural levels, respectively. (c-f) Uncertainty estimates for GRACE-FS-M using (c, d) ensemble learning and (e, f) the D-optimality criterion, each shown at the atomic and structural level.
  • Figure 3: Computational speed comparison between UNEP-v1 and GRACE-FS-M for (a) pure Cu and (b) the Al$_{31}$Cr$_{6}$Cu$_{22}$Ni$_{32}$V$_{9}$ HEA. UNEP-v1 is evaluated on A100 and H100 GPUs, while GRACE-FS-M is run on 192 CPU cores.
  • Figure 4: Thermal stability of goldene assessed by MD simulations. (a) Maximum energy drift as a function of temperature. (b, c) Atomic snapshots of the structure after relaxation at 1,500 K, showing the different structures obtained by two MLIPs at extreme conditions.
  • Figure 5: Assessing the thermal stability of HEAs via MD simulations. The maximum energy drift, a key metric for stability, is plotted for (a) the Al$_{31}$Cr$_{6}$Cu$_{22}$Ni$_{32}$V$_{9}$ alloy with chemical short-range order (CSRO) and (b) a random 16-element alloy across a range of temperatures.
  • ...and 5 more figures