Correlation energy of the paramagnetic electron gas at the thermodynamic limit
arXiv:2209.10227 · doi:10.1103/PhysRevB.107.L121105
Abstract
The variational and diffusion quantum Monte Carlo methods are used to calculate the correlation energy of the paramagnetic three-dimensional homogeneous electron gas at intermediate to high density. Ground state energies in finite cells are determined using Slater-Jastrow-backflow trial wave functions, and finite-size errors are removed using twist-averaged boundary conditions and extrapolation of the energy per particle to the thermodynamic limit of infinite system size. Our correlation energies in the thermodynamic limit are lower (i.e., more negative, and therefore more accurate according to the variational principle) than previous results, and can be used for the parameterization of density functionals to be applied to high-density systems.
References in corpus (9)
- Inhomogeneous backflow transformations in quantum Monte Carlo calculations
- The Finite Size Error in Many-body Simulations with long-Ranged Interactions
- {\em Ab initio} Quantum Monte Carlo simulation of the warm dense electron gas in the thermodynamic limit
- Resonating valence bond wave function with molecular orbitals: Application to first-row molecules
- Discovering Quantum Phase Transitions with Fermionic Neural Networks
- Low-density Phase Diagram of the Three-Dimensional Electron Gas
- Correlation energy of the spin-polarized uniform electron gas at high density
- An efficient method for grand-canonical twist averaging in quantum Monte Carlo calculations
- Quasiparticle Effective Mass of the Three-Dimensional Fermi Liquid by Quantum Monte Carlo
Cited by in corpus (4)
- Message-Passing Neural Quantum States for the Homogeneous Electron Gas
- Quantum Monte Carlo study of the phase diagram of the two-dimensional uniform electron liquid
- Energy response and spatial alignment of the perturbed electron gas
- Correlation energy of the spin-polarized electron liquid by quantum Monte Carlo