Uniform electron gas at finite temperatures

Abstract

We calculate the free energy of the quantum uniform electron gas for temperatures from near zero to 100 times the Fermi energy, approaching the classical limit. An extension of the Vashista-Singwi theory to finite temperatures and self-consistent compressibility sum rule is presented. Comparisons are made to other local field correction methods, as well as recent quantum Monte Carlo simulation and classical map based results. Accurate fits to the exchange-correlation free energy from both theory and simulation are given for future practical applications.

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• Path Integral Monte Carlo Simulation of the Warm-Dense Homogeneous Electron Gas
• All-Electron Path Integral Monte Carlo Simulations of Warm Dense Matter: Application to Water and Carbon Plasmas
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Cited by in corpus (49)

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• Finite-size effects in the reconstruction of dynamic properties from ab initio path integral Monte-Carlo simulations
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