Virial equation of state: Difference between revisions

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where ''f'' is the [[Mayer f-function]] (see also: [[Cluster integrals]]).
where ''f'' is the [[Mayer f-function]] (see also: [[Cluster integrals]]).
See also:
*[http://dx.doi.org/10.1080/002689796173453 M. S. Wertheim "Fluids of hard convex molecules III. The third virial coefficient", Molecular Physics '''89''' pp. 1005-1017 (1996)]
==Convergence==
==Convergence==
See Ref. 3.
See Ref. 3.

Revision as of 13:08, 30 August 2007

The virial equation of state is used to describe the behavior of diluted gases. It is usually written as an expansion of the compressibility factor, Z, in terms of either the density or the pressure. Such an expansion was first introduced by Kammerlingh Onnes. In the first case:

pVNkBT=Z=1+∑k=2∞Bk(T)ρk−1.

where

  • p is the pressure
  • V is the volume
  • N is the number of molecules
  • ρ≡NV is the (number) density
  • Bk(T) is called the k-th virial coefficient

Virial coefficients

The second virial coefficient represents the initial departure from ideal-gas behavior

B2(T)=N02V∫....∫(1−e−Φ/kBT)dτ1dτ2

where N0 is Avogadros number and dτ1 and dτ2 are volume elements of two different molecules in configuration space.

One can write the third virial coefficient as

B3(T)=−13V∫∫∫f12f13f23dr1dr2dr3

where f is the Mayer f-function (see also: Cluster integrals). See also:

Convergence

See Ref. 3.

References

  1. H. Kammerlingh Onnes "", Communications from the Physical Laboratory Leiden 71 (1901)
  2. James A Beattie and Walter H Stockmayer "Equations of state", Reports on Progress in Physics 7 pp. 195-229 (1940)
  3. J. L. Lebowitz and O. Penrose "Convergence of Virial Expansions", Journal of Mathematical Physics 5 pp. 841-847 (1964)