Deep Variational Free Energy Calculation of Hydrogen Hugoniot
Zihang Li, Hao Xie, Xinyang Dong, Lei Wang
TL;DR
This work introduces a deep variational free-energy framework to compute the equation of state and Hugoniot of hydrogen in the warm dense matter regime by jointly optimizing three neural models: a normalizing flow for nuclear Boltzmann sampling, a masked autoregressive network for finite-temperature electronic excitations, and a quantum flow-based transformation of Hartree-Fock states to form the electronic wavefunctions. The approach enables finite-temperature, excited-state electronic effects to be incorporated into a variational density-matrix, circumventing the fermion sign problem and connecting finite-temperature methods with ground-state calculations. Results for deuterium across multiple system sizes, densities, and temperatures show sensible agreement with experimental data and other theories, while providing insight into electron occupation, RDFs, and the role of temperature in dissociation and metallization processes. The method offers a robust benchmark for EOS in the WDM region and a path toward consistent cross-regime predictions crucial for planetary modeling and inertial confinement fusion.
Abstract
We develop a deep variational free energy framework to compute the equation of state of hydrogen in the warm dense matter region. This method parameterizes the variational density matrix of hydrogen nuclei and electrons at finite temperature using three deep generative models: a normalizing flow model for the Boltzmann distribution of the classical nuclei, an autoregressive transformer for the distribution of electrons in excited states, and a permutational equivariant flow model for the unitary backflow transformation of electron coordinates in Hartree-Fock states. By jointly optimizing the three neural networks to minimize the variational free energy, we obtain the equation of state and related thermodynamic properties of dense hydrogen for the temperature range where electrons occupy excited states. We compare our results with other theoretical and experimental results on the deuterium Hugoniot curve, aiming to resolve existing discrepancies. Our results bridge the gap between the results obtained by path-integral Monte Carlo calculations at high temperature and ground-state electronic methods at low temperature, thus providing a valuable benchmark for hydrogen in the warm dense matter region.
