Carnahan-Starling equation of state: Difference between revisions
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The equation of Carnahan-Starling is an | The equation of Carnahan-Starling is an approximate equation of state for the fluid phase of the [[Hard Sphere]] model in three dimensions. | ||
: <math> | |||
Z = \frac{ p V}{N k_B T} = \frac{ 1 + \eta + \eta^2 - \eta^3 }{(1-\eta)^3 }. | |||
</math> | |||
where: | |||
* <math> p </math> is the pressure | |||
*<math> V </math> is the volume | |||
*<math> N </math> is the number of particles | |||
*<math> k_B </math> is the [[Boltzmann]] constant | |||
*<math> T </math> is the absolute temperature | |||
*<math> \eta </math>, is the packing fraction: | |||
:<math> \eta = \frac{ \pi }{6} \frac{ N \sigma^3 }{V} </math> | |||
A reference is required here (please check) |
Revision as of 18:59, 16 February 2007
The equation of Carnahan-Starling is an approximate equation of state for the fluid phase of the Hard Sphere model in three dimensions.
where:
- is the pressure
- is the volume
- is the number of particles
- is the Boltzmann constant
- is the absolute temperature
- , is the packing fraction:
A reference is required here (please check)