Integral equation model for warm and hot dense mixtures

C. E. Starrett, D. Saumon, J. Daligault, and S. Hamel
Phys. Rev. E 90, 033110 – Published 19 September 2014

Abstract

In a previous work [C. E. Starrett and D. Saumon, Phys. Rev. E 87, 013104 (2013)] a model for the calculation of electronic and ionic structures of warm and hot dense matter was described and validated. In that model the electronic structure of one atom in a plasma is determined using a density-functional-theory-based average-atom (AA) model and the ionic structure is determined by coupling the AA model to integral equations governing the fluid structure. That model was for plasmas with one nuclear species only. Here we extend it to treat plasmas with many nuclear species, i.e., mixtures, and apply it to a carbon-hydrogen mixture relevant to inertial confinement fusion experiments. Comparison of the predicted electronic and ionic structures with orbital-free and Kohn-Sham molecular dynamics simulations reveals excellent agreement wherever chemical bonding is not significant.

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  • Received 14 August 2014

DOI:https://doi.org/10.1103/PhysRevE.90.033110

©2014 American Physical Society

Authors & Affiliations

C. E. Starrett, D. Saumon, and J. Daligault

  • Los Alamos National Laboratory, P.O. Box 1663, Los Alamos, New Mexico 87545, USA

S. Hamel

  • Lawrence Livermore National Laboratory, Livermore, California 94550, USA

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Issue

Vol. 90, Iss. 3 — September 2014

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