Improving Kubo-Greenwood Conductivity Predictions with the GW Approximation
ORAL
Abstract
Simulations of high-energy-density (HED) experiments often rely on the resistive magnetohydrodynamic equations, which require parameters like the DC electrical conductivity for closure.
State-of-the-art conductivity calculations for warm dense matter typically evaluate the Kubo-Greenwood (KG) equation using Kohn-Sham energies and wavefunctions from density functional theory (DFT). In this work, we present a first-principles approach for improving the accuracy of KG conductivities through many-body perturbation theory. We use the GW approximation to compute the complex electron self-energy, where the real part gives the quasiparticle (qp) energies and the imaginary part the qp lifetimes. We then modify the KG equation by replacing the DFT eigenvalues and occupations with the corresponding GW values. Further, we replace the commonly used ad hoc static broadening factor with a dynamic form governed by the qp lifetimes, resulting in a more accurate description of the broadening effects. Throughout, we demonstrate our approach for both non-thermalized and thermalized warm dense beryllium near solid density and at temperatures up to 7 eV. By improving the electron correlation description, we expect the GW approximation to improve the accuracy of the KG conductivity predictions, thus leading to more accurate modeling of HED experiments.
*SNL is managed and operated by NTESS under DOE NNSA contract DE-NA0003525.
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Presenters
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Brian Robinson
- University of Illinois Urbana-Champaign