Pair distribution function of the spin-polarized electron gas: A first-principles analytic model for all uniform densities
arXiv:cond-mat/0206147 · doi:10.1103/PhysRevB.66.165118
Abstract
We construct analytic formulas that represent the coupling-constant-averaged pair distribution function $\gxcav(r_s,ζ, k_Fu)$ of a uniform electron gas with density parameter and relative spin polarization over the whole range and , with energetically-unimportant long range () oscillations averaged out. The pair distribution function at the physical coupling constant is then given by differentiation with respect to . Our formulas are constructed using {\em only} known theoretical constraints plus the correlation energy $\ec(r_s,ζ)$, and accurately reproduce the of the Quantum Monte Carlo method and of the fluctuation-dissipation theorem with the Richardson-Ashcroft dynamical local-field factor. Our seems to be correct even in the high-density () and low-density () limits. When the spin resolution of $\ec$ into $\uu$, $\dd$, and $\ud$ contributions is known, as it is in the high- and low-density limits, our formulas also yield the spin resolution of . We also analyze the kinetic energy of correlation into contributions from density fluctuations of various wavevectors.
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