Virial expansion

The classical virial expansion expresses the pressure of a many-particle system in equilibrium as a power series in the density. The virial expansion was introduced in 1901 by Heike Kamerlingh Onnes as a generalization of the ideal gas law. He wrote for a gas containing N atoms or molecules,


   \frac{p}{k_BT} = \rho %2B B_2(T) \rho^2 %2BB_3(T) \rho^3%2B \cdots,

where p is the pressure, k_B is the Boltzmann constant, T is the absolute temperature, and \rho \equiv N/V is the number density of the gas. Note that for a gas containing a fraction n of N_A (Avogadro's number) molecules, truncation of the virial expansion after the first term leads to pV = n N_A k_B T = nRT, which is the ideal gas law.

Writing \beta=(k_{B}T)^{-1}, the virial expansion can be written in closed form as

\frac{\beta p}{\rho}=1%2B\sum_{i=1}^{\infty}B_{i%2B1}(T)\rho^{i}.

The virial coefficients B_i(T) are characteristic of the interactions between the particles in the system and in general depend on the temperature T.

See also

Statistical mechanics