Carnahan-Starling equation of state

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CS EoS plot.png

The Carnahan-Starling equation of state is an approximate (but quite good) equation of state for the fluid phase of the hard sphere model in three dimensions. It is given by (Ref [1] Eqn. 10).


Z = \frac{ p V}{N k_B T} = \frac{ 1 + \eta + \eta^2 - \eta^3 }{(1-\eta)^3 }.

where:

 \eta = \frac{ \pi }{6} \frac{ N \sigma^3 }{V}

The Carnahan-Starling equation of state is not applicable for packing fractions greater than 0.55 [2].

Virial expansion[edit]

It is interesting to compare the virial coefficients of the Carnahan-Starling equation of state (Eq. 7 of [1]) with the hard sphere virial coefficients in three dimensions (exact up to B_4, and those of Clisby and McCoy [3]):

n Clisby and McCoy B_n=n^2+n-2
2 4 4
3 10 10
4 18.3647684 18
5 28.224512 28
6 39.8151475 40
7 53.3444198 54
8 68.5375488 70
9 85.8128384 88
10 105.775104 108

Thermodynamic expressions[edit]

From the Carnahan-Starling equation for the fluid phase the following thermodynamic expressions can be derived (Ref [4] Eqs. 2.6, 2.7 and 2.8)

Pressure (compressibility):

\frac{p^{CS}V}{N k_B T } = \frac{1+ \eta + \eta^2 - \eta^3}{(1-\eta)^3}


Configurational chemical potential:

\frac{ \overline{\mu }^{CS}}{k_B T} = \frac{8\eta -9 \eta^2 + 3\eta^3}{(1-\eta)^3}

Isothermal compressibility:

\chi_T -1 = \frac{1}{k_BT} \left.\frac{\partial P^{CS}}{\partial \rho}\right\vert_{T} -1 =   \frac{8\eta -2 \eta^2 }{(1-\eta)^4}

where \eta is the packing fraction.

Configurational Helmholtz energy function:

 \frac{ A_{ex}^{CS}}{N k_B T}  = \frac{4 \eta - 3 \eta^2 }{(1-\eta)^2}

The 'Percus-Yevick' derivation[edit]

It is interesting to note (Ref [5] Eq. 6) that one can arrive at the Carnahan-Starling equation of state by adding two thirds of the exact solution of the Percus Yevick integral equation for hard spheres via the compressibility route, to one third via the pressure route, i.e.

Z = \frac{ p V}{N k_B T} =  \frac{2}{3} \left[   \frac{(1+\eta+\eta^2)}{(1-\eta)^3}  \right] +  \frac{1}{3} \left[     \frac{(1+2\eta+3\eta^2)}{(1-\eta)^2}  \right] = \frac{ 1 + \eta + \eta^2 - \eta^3 }{(1-\eta)^3 }

The reason for this seems to be a slight mystery (see discussion in Ref. [6] ).

Kolafa correction[edit]

Jiri Kolafa produced a slight correction to the C-S EOS which results in improved accuracy [7]:


Z =  \frac{ 1 + \eta + \eta^2 -  \frac{2}{3}(1+\eta) \eta^3 }{(1-\eta)^3 }.

See also[edit]

References[edit]