Carnahan-Starling equation of state: Difference between revisions
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*<math> N </math> is the number of particles | *<math> N </math> is the number of particles | ||
*<math> k_B </math> is the [[ | *<math> k_B </math> is the [[Boltzmann constant]] | ||
*<math> T </math> is the absolute temperature | *<math> T </math> is the absolute temperature | ||
*<math> \eta </math> is the packing fraction: | *<math> \eta </math> is the [[packing fraction]]: | ||
:<math> \eta = \frac{ \pi }{6} \frac{ N \sigma^3 }{V} </math> | :<math> \eta = \frac{ \pi }{6} \frac{ N \sigma^3 }{V} </math> | ||
*<math> \sigma </math> is the [[ | *<math> \sigma </math> is the [[hard sphere]] diameter. | ||
== References == | == References == |
Revision as of 12:45, 21 March 2007
The equation of Carnahan-Starling is an approximate equation of state for the fluid phase of the hard sphere model in three dimensions. (Eqn. 10 in Ref 1).
where:
- is the pressure
- is the volume
- is the number of particles
- is the Boltzmann constant
- is the absolute temperature
- is the packing fraction:
- is the hard sphere diameter.