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Ion model of a hot dense plasma

Published online by Cambridge University Press:  09 March 2009

N.Y. Orlov
Affiliation:
Institute of Mathematical Modelling, 4-A Miusskaya Square, 125047, Moscow, Russia

Abstract

Results are presented for a theoretical model, known as the ion model (IM), recently elaborated to calculate the radiative opacity of a hot dense plasma. The model is based on the self-consistent field method for subsystems obeying Gibbs statistics. The results are compared with calculations that use the Hartree-Fock-Slater model and with experimental data. A theory is proposed to explain the extraordinary spectral line-shift phenomenon associated with such plasmas.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1997

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