Equation of state and opacity of dense plasmas

Details Equation of state and opacity of dense plasmas Equation of state and opacity of dense plasmas

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989scpp.conf.....r&link_type=abstract

Presented at the 24th Yamada Conference on Strongly Coupled Plasma Physics, Tokyo, Japan, 29 Aug. - 2 Sep. 1989

Statistics

Computation

2

Dense Plasmas, Equations Of State, Opacity, Star Clusters, Variable Stars, Computation, Excitation, Lithium

Scientific paper

Recent research on the equation of state and opacity of dense plasmas has been strongly driven by discrepancies between calculation and observation of a wide variety of astrophysical quantities such as the solar neutrino flux rate, the period ratio of Cepheid variable stars, and lithium depletion in the Hyades stellar cluster. A summary of some recent work based on a many-body activity expansion of the grand-partition function is given. An integral part of this work involves methods for calculating atomic data and occupation numbers for excited states in dense plasmas.

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