Matter and Radiation at Extremes, Volume. 9, Issue 1, 015604(2024)
Combining stochastic density functional theory with deep potential molecular dynamics to study warm dense matter
Fig. 1. Workflow of the simulation of WDM with the SDFT and DPMD methods. (a) Stochastic orbitals are employed in SDFT to perform molecular dynamics simulations on smaller systems (32 atoms in a bulk B) and initial training data are collected that include atomic positions, energies, forces, and virial tensors. (b) The gathered training data are used to construct a DP model with the temperature-dependent DPMD model. The deep neural network contains both embedding and fitting networks. (c) The new model enables simulations to be performed on large systems (16 384 atoms) and at extremely high temperatures (350 eV). (d) Several physical quantities such as radial distribution functions, static structure factors, dynamic structure factors, and shear viscosities can be calculated, and the data are converged with large systems and long trajectories.
Fig. 2. Root-mean-square error (RMSE) of atomic forces arising from the SDFT calculations for B. The temperature is set to 350 eV and the density to 2.46 g/cm3. The RMSE is evaluated with respect to (a) the number of stochastic orbitals
Fig. 3. Forces acting on each B atom as obtained from nine independent SDFT calculations with different stochastic orbitals. The B system has a density of 2.46 g/cm3, and the temperature is 17.23 eV. For each calculation, the force acting on each atom along the
Fig. 4. (a) Comparison of forces acting on each B atom in a 32-atom cell for densities of 2.46 and 12.3 g/cm3 at a temperature of 17.23 eV. (b) Comparison of forces acting on each C atom for densities of 4.17 and 12.46 g/cm3 at a temperature of 21.54 eV. In the SDFT and KSDFT calculations, we denote the forces acting on each atom along the
Fig. 5. DOS for the B and C systems as calculated by the SDFT and KSDFT methods. The densities are selected as (a) 2.46 g/cm3 and (b) 12.3 g/cm3 for the B system, and (c) 4.17 g/cm3 and (d) 12.64 g/cm3 for the C system. The Fermi energy is set to zero. We use two sets of
Fig. 6. Radial distribution functions
Fig. 7. Static structure factors
Fig. 8. Intermediate scattering functions
Fig. 9. Ion–ion dynamic structure factors
Fig. 10. Stress autocorrelation functions [Eq.
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Tao Chen, Qianrui Liu, Yu Liu, Liang Sun, Mohan Chen. Combining stochastic density functional theory with deep potential molecular dynamics to study warm dense matter[J]. Matter and Radiation at Extremes, 2024, 9(1): 015604
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Received: Jun. 16, 2023
Accepted: Dec. 13, 2023
Published Online: Mar. 27, 2024
The Author Email: Chen Mohan (mohanchen@pku.edu.cn)