Equation of state, transport coefficients, and stopping power of dense plasmas from the average-atom model self-consistent approach for astrophysical and laboratory plasmas

Details Equation of state, transport coefficients, and stopping power of dense plasmas from the average-atom model self-consistent approach for astrophysical and laboratory plasmas Equation of state, transport coefficients, and stopping power of dense plasmas from the average-atom model self-consistent approach for astrophysical and laboratory plasmas

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010phpl...17e2707f&link_type=abstract

Physics of Plasmas, Volume 17, Issue 5, pp. 052707-052707-11 (2010).

Physics

13

Density Functional Theory, Molecular Dynamics Method, Monte Carlo Methods, Plasma Density, Plasma Transport Processes, Thermodynamic Functions And Equations Of State, Transport Processes, Particle Beam Interactions In Plasmas

Scientific paper

Calculations of equation of state, transport coefficients, and stopping power of dense plasmas are presented. Theoretical results have been obtained using the first-principles average-atom model self-consistent approach for astrophysical and laboratory plasmas (SCAALP) based on the finite-temperature density-functional theory and the Gibbs-Bogolyubov inequality. Numerical results, comparisons with molecular dynamics, and Monte Carlo simulations and experiments are presented and discussed in the high energy density physics domain including part of the warm dense matter regime. Results show that the average-atom model SCAALP is well suited to describe thermodynamic and transport properties for a wide range of high energy density physics applications.

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