To use all functions of this page, please activate cookies in your browser.
With an accout for my.chemeurope.com you can always see everything at a glance – and you can configure your own website and individual newsletter.
- My watch list
- My saved searches
- My saved topics
- My newsletter
Virial coefficients Bi appear as coefficients in the virial expansion of the pressure of a many-particle system in powers of the density. They are characteristic of the interaction potential between the particles and in general depend on the temperature. The second virial coefficient B2 depends only on the pair interaction between the particles, the third (B3) depends on 2- and non-additive 3-body interactions, and so on.
Additional recommended knowledge
Here p is the pressure, V is the volume of the vessel containing the particles, kB is Boltzmann's constant, T is the absolute temperature, λ = exp[μ / (kBT)], with μ the chemical potential. The quantity Qn is the canonical partition function of a subsystem of n particles:
Here is the Hamiltonian (energy operator) of a subsystem of n particles. The Hamiltonian is a sum of the kinetic energies of the particles and the total n-particle potential energy (interaction energy). The latter includes pair interactions and possibly 3-body and higher-body interactions. The grand partition function Ξ can be expanded in a sum of contributions from one-body, two-body, etc. clusters. The virial expansion is obtained from this expansion by observing that lnΞ equals pV / (kBT). In this manner one derives
These are quantum-statistical expressions containing kinetic energies. Note that the one-particle partition function Q1 contains only a kinetic energy term. In the classical limit the kinetic energy operators commute with the potential operators and the kinetic energies in numerator and denominator cancel mutually. The trace (tr) becomes an integral over the configuration space. It follows that classical virial coefficients depend on the interactions between the particles only and are given as integrals over the particle coordinates.
The derivation of higher than B3 virial coefficients becomes quickly a complex combinatorial problem. Making the classical approximation and neglecting non-additive interactions (if present), the combinatorics can be handled graphically as first shown by Joseph E. Mayer and Maria Goeppert-Mayer . They introduced the function
and wrote the cluster expansion in terms of these functions. Here is the interaction between particle 1 and 2 (which are assumed to be identical particles).
Definition in terms of graphs
The virial coeffcients Bi are related to the irreducible Mayer cluster integrals βi through
The rule for turning these graphs into integrals is as follows:
The first two cluster integrals are
In particular we get
where particle 2 was assumed to define the origin (). This classical expression for the second virial coefficient was first derived by L. S. Ornstein in his 1908 Leiden University Ph.D. thesis.
Boyle temperature - temperature at which the second virial coefficient B2 vanishes
|This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Virial_coefficient". A list of authors is available in Wikipedia.|