Liu hard sphere equation of state: Difference between revisions
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Hongqin Liu proposed a correction to the | Hongqin Liu proposed a correction to the [[Carnahan-Starling equation of state]] which improved accuracy by almost two orders of magnitude <ref>[https://arxiv.org/abs/2010.14357 Hongqin Liu "Carnahan Starling type equations of state for stable hard disk and hard sphere fluids", arXiv:2010.14357]</ref>: | ||
: <math> | : <math> | ||
Z = \frac{ 1 + \eta + \eta^2 - \frac{8}{13}\eta^3 - \eta^4 + \frac{1}{2}\eta^5 }{(1-\eta)^3 }. | Z = \frac{ 1 + \eta + \eta^2 - \frac{8}{13}\eta^3 - \eta^4 + \frac{1}{2}\eta^5 }{(1-\eta)^3 }. | ||
</math> | </math> | ||
The conjugate [[Virial equation of state | virial coefficient]] correlation is given by: | |||
: <math> | |||
B_n = 0.9423n^2 + 1.28846n - 1.84615, n > 3. | |||
</math> | |||
The excess [[Helmholtz energy function]] is given by: | |||
: <math> | |||
A^{ex} = \frac{ A - A^{id}}{Nk_B}= \frac{ 188\eta - 126\eta^2 - 13\eta^4 }{52(1-\eta)^2} - \frac{5}{13} ln(1-\eta). | |||
</math> | |||
The isothermal [[compressibility]] is given by: | |||
: <math> | |||
k_T = (\eta\frac{ dZ}{d\eta} + Z)^{-1} \rho^{-1}. | |||
</math> | |||
where | |||
: <math> | |||
\frac{ dZ}{d\eta} = \frac{ 4 + 4\eta - \frac {11}{13} \eta^2 - \frac{52}{13}\eta^3 + \frac {7}{2}\eta^4 - \eta^5 }{(1-\eta)^4 }. | |||
</math> | |||
== References == | |||
<references/> | |||
[[Category: Equations of state]] | |||
[[category: hard sphere]] |
Latest revision as of 11:21, 10 November 2020
Hongqin Liu proposed a correction to the Carnahan-Starling equation of state which improved accuracy by almost two orders of magnitude [1]:
The conjugate virial coefficient correlation is given by:
The excess Helmholtz energy function is given by:
The isothermal compressibility is given by:
where