Plasma Physics
DOI: 10.1007/11360360_12
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Plasmas in Planetary Interiors

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Cited by 2 publications
(2 citation statements)
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“…The excluded volume concept is one of the popular simpler approximations to take the interaction of electrons with neutrals into account [31]. The fraction of volume occupied by atoms can be defined with the filling parameter η = 4/3πr 3 H n H , where r H is an atomic radius. The second virial coefficient is given for a system of hard spheres as…”
Section: Comparison With the Excluded Volume Approachmentioning
confidence: 99%
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“…The excluded volume concept is one of the popular simpler approximations to take the interaction of electrons with neutrals into account [31]. The fraction of volume occupied by atoms can be defined with the filling parameter η = 4/3πr 3 H n H , where r H is an atomic radius. The second virial coefficient is given for a system of hard spheres as…”
Section: Comparison With the Excluded Volume Approachmentioning
confidence: 99%
“…The equation of state describing fundamental characteristics of matter attracts significant attention of researchers from multiple disciplines. For instance, the calculation of thermodynamic properties of plasmas in the warm dense matter region is necessary to solve problems of high energy density physics [1] and to model the planetary and stellar interiors [2,3]. Correlations and bound state formation are of relevance since simple treatment of plasma using perturbation methods is not possible in this region.…”
Section: Introductionmentioning
confidence: 99%