APS Logo

Melting line of dense hydrogen from hierarchical machine learning using diffusion Monte Carlo data

ORAL

Abstract

The phase transitions of dense hydrogen are of interest in astrophysics and in condensed matter physics. Ab initio simulations suffer from errors due to small system sizes, while empirical potentials lack the accuracy needed to describe these transitions. To minimize these errors, we use diffusion Monte Carlo (DMC) forces to train a hierarchical machine-learning potential and perform large-scale two-phase classical molecular dynamics and quantum path integral molecular dynamics simulations to estimate the melting line for dense hydrogen in the pressure range 50-200 GPa. We estimate the effect on the melting temperature coming from the assumed density functional, from the machine-learning procedures, and from the nuclear zero-point motion.

Presenters

  • Hongwei Niu

    Department of Astronautical Science and Mechanics, Harbin Institute of Technology

Authors

  • Hongwei Niu

    Department of Astronautical Science and Mechanics, Harbin Institute of Technology

  • Yubo Yang

    Department of Physics, University of Illinois

  • Scott Jensen

    University of Illinois at Urbana-Champaign, Department of Physics, University of Illinois

  • Markus Holzmann

    Univ. Grenoble Alpes

  • CARLO PIERLEONI

    University of L’Aquila, Maison de la Simulation, CEA, CNRS, Univ. Paris-Sud,UVSQ, Université Paris-Saclay, 91191 Gif-sur-Yvette, France, Department of Physical and Chemical Sciences, University of L, Department of Physical and Chemical Sciences, University of L'Aquila

  • David M Ceperley

    University of Illinois at Urbana-Champaign, Department of Physics, University of Illinois, Urbana, Illinois 61801, USA, Department of Physics, University of Illinois