Correlation and prediction of thermodynamic properties of dilute solutes in water up to high T and P. I. Simple fluids He, Ne, Ar, Kr, Xe, Rn, H2, N2, O2, CO, CH4

By using the properties of hard-sphere systems as a point of departure, equations are derived for the residual properties of mixtures of real simple fluids at liquid-like densities. The essence of the derivation lies in a functional expansion of g(r) exp [Formula: see text] about its hard-sphere value. The results obtained are useful for interpreting, correlating, and extending experimental data for both concentrated and dilute liquid solutions.

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Calculation of thermodynamic properties of simple fluids using a new derived pair correlation function

Fluid Phase Equilibria ◽

10.1016/j.fluid.2007.03.005 ◽

2007 ◽

Vol 254 (1-2) ◽

pp. 138-143 ◽

Cited By ~ 1

Author(s):

Mehrdad Khanpour ◽

G.A. Parsafar ◽

B. Najafi

Keyword(s):

Correlation Function ◽

Thermodynamic Properties ◽

Pair Correlation Function ◽

Pair Correlation ◽

Simple Fluids

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Calculation of density fluctuation contributions to thermodynamic properties of simple fluids

The Journal of Chemical Physics ◽

10.1063/1.462791 ◽

1992 ◽

Vol 96 (6) ◽

pp. 4559-4568 ◽

Cited By ~ 65

Author(s):

Liming W. Salvino ◽

John A. White

Keyword(s):

Thermodynamic Properties ◽

Density Fluctuation ◽

Simple Fluids

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Monte Carlo Calculation of Thermodynamic Properties of Simple Fluids

Nature ◽

10.1038/2121449a0 ◽

1966 ◽

Vol 212 (5069) ◽

pp. 1449-1449 ◽

Cited By ~ 3

Author(s):

K. SINGER

Keyword(s):

Monte Carlo ◽

Thermodynamic Properties ◽

Monte Carlo Calculation ◽

Simple Fluids

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Models of Thermodynamic Properties of Prominences

International Astronomical Union Colloquium ◽

10.1017/s0252921100065799 ◽

1979 ◽

Vol 44 ◽

pp. 349-355

Author(s):

R.W. Milkey

Keyword(s):

Thermodynamic Properties ◽

Mass Transport ◽

Emission Spectrum ◽

Thermodynamic Parameters ◽

Working Group ◽

Physical Processes ◽

Theoretical Concepts ◽

Group 3 ◽

Observational Techniques

The focus of discussion in Working Group 3 was on the Thermodynamic Properties as determined spectroscopically, including the observational techniques and the theoretical modeling of physical processes responsible for the emission spectrum. Recent advances in observational techniques and theoretical concepts make this discussion particularly timely. It is wise to remember that the determination of thermodynamic parameters is not an end in itself and that these are interesting chiefly for what they can tell us about the energetics and mass transport in prominences.

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