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Path Integral Monte Carlo Simulation of the Warm-Dense Homogeneous Electron Gas

Published 26 Nov 2012 in cond-mat.str-el and cond-mat.other | (1211.6130v2)

Abstract: We perform calculations of the {3D} finite-temperature homogeneous electron gas (HEG) in the warm-dense regime ({r_{s} \equiv (3/4\pi n){1/3}a_{B}{- 1} = 1.0- 40.0} and {\Theta \equiv T/T_{F} = 0.0625- 8.0}) using restricted path integral Monte Carlo (RPIMC). Precise energies, pair correlation functions, and structure factors are obtained. For all densities, we find a significant discrepancy between the ground state parameterized local density approximation (LDA) and our results around {T_{F}} . These results can be used as a benchmark for improved functionals, as well as input for orbital-free DFT formulations.

Citations (176)

Summary

Path Integral Monte Carlo Simulation of the Warm-Dense Homogeneous Electron Gas

The paper presents a detailed analysis of the three-dimensional finite-temperature homogeneous electron gas (HEG) within the warm-dense regime utilizing the Restricted Path Integral Monte Carlo (RPIMC) method. This study examines electron gas properties, bridging previous ground-state studies and classical simulations under conditions where both quantum and classical behaviors coexist.

The authors focus on calculating precise thermodynamic quantities for the HEG across various densities and temperatures. They investigate the Wigner-Seitz radius ( r_{s} = 1.0-40.0 ), and the degeneracy parameter ( \Theta = T/T_{F} = 0.0625-8.0 ). The research deviates from ground state parameterized local density approximation (LDA) results near the Fermi temperature, posing significant implications for density functional theory (DFT), especially in the context of finite-temperature systems such as stellar interiors and dense plasmas.

The application of RPIMC is notable due to its ability to address equilibrium properties of quantum systems, overcoming challenges like the fermion sign problem through constrained path sampling. A key innovation is the use of free-electron density matrix nodes to approximate trial paths, a technique that yields high accuracy, particularly at higher temperatures and lower densities.

Key numerical outcomes include:

  • Excess Energy Calculation: Across various ( r_s ), the excess energy results deviate from classical Monte Carlo data at lower values of ( \Theta ), signifying quantum effects are prominent in these conditions. The results smoothly extrapolate to zero-temperature limits aligning with Ceperley-Alder ground-state QMC data.
  • Structural Factors: The paper presents calculated structure factors for the unpolarized HEG states, displaying convergence with classical Debye-Huckel limits as temperature increases.
  • Pair Correlation Functions: The study highlights pair correlation function deviations due to quantum mechanical integration, particularly at smaller ( r ).

The authors discuss implications for finite-temperature DFT, emphasizing that the calculated exchange-correlation energies could enhance the parameterization of temperature-dependent density functionals. The RPIMC methodology sets a benchmark for future DFT functional enhancements, ensuring more reliable simulations of correlated electron systems across various regimes.

Theoretical implications suggest that further refinement of nodal structures could reduce RPIMC bias in higher density and lower temperature scenarios. This research underlines the necessity for improved DFT functionals addressing significant electron correlations in warm-dense conditions.

Given these advancements, future directions may include investigating ultra-high-density and low-temperature conditions where RPIMC node approximations might falter, alongside algorithmic innovations to enhance path sampling efficacy.

In conclusion, this paper contributes comprehensive simulation data poised to aid the development of more robust finite-temperature DFT frameworks, which are crucial for addressing modern challenges in computational condensed matter physics.

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