高温下的均匀电子气体:从头算路径积分蒙特卡罗模拟和分析理论

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS High Energy Density Physics Pub Date : 2022-12-01 DOI:10.1016/j.hedp.2022.101015
Tobias Dornheim , Jan Vorberger , Zhandos Moldabekov , Gerd Röpke , Wolf-Dietrich Kraeft
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引用次数: 12

摘要

本文对均匀电子气体(UEG)在高温条件下进行了广泛的新的从头算路径积分蒙特卡罗(PIMC)模拟,8≤θ=kBT/EF≤128。这使我们能够研究不同性质在经典极限下的收敛性。特别地,我们研究了静态结构因子S(q)与静态局部场校正G(q)之间的经典关系,这种关系仅在低密度下实现。此外,我们将相互作用能的新结果与growth等人(2017)对UEG的参数化进行了比较,后者在θ≤8的PIMC结果和debye - hckel极限之间进行了插值,并与高阶解析维里展开进行了比较。最后,我们考虑动量分布函数n(q),并发现即使在θ≥32时,相互作用也会导致零动量态占据的增加。所有的PIMC数据都可以在网上免费获得,可以用作改进参数化的输入,也可以作为近似方法的严格基准。
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The uniform electron gas at high temperatures: ab initio path integral Monte Carlo simulations and analytical theory

We present extensive new Ab initio path integral Monte Carlo (PIMC) simulations of the uniform electron gas (UEG) in the high-temperature regime, 8θ=kBT/EF128. This allows us to study the convergence of different properties towards the classical limit. In particular, we investigate the classical relation between the static structure factor S(q) and the static local field correction G(q), which is only fulfilled at low densities. Moreover, we compare our new results for the interaction energy to the parametrization of the UEG by Groth et al. (2017), which interpolates between PIMC results for θ8 and the Debye–Hückel limit, and to higher order analytical virial expansions. Finally, we consider the momentum distribution function n(q) and find an interaction-induced increase in the occupation of the zero-momentum state even for θ32. All PIMC data are freely available online, and can be used as input for improved parametrizations and as a rigorous benchmark for approximate methods.

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来源期刊
High Energy Density Physics
High Energy Density Physics PHYSICS, FLUIDS & PLASMAS-
CiteScore
4.20
自引率
6.20%
发文量
13
审稿时长
6-12 weeks
期刊介绍: High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings. Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.
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