For a fluid of
particles, enclosed in a volume
at a given temperature
(canonical ensemble) interacting via the `central' potential
, the two particle distribution function is defined as

Exact convolution equation for 
See Eq. 5.10 of Ref. 1:

See also
References
- J. S. Rowlinson "The equation of state of dense systems", Reports on Progress in Physics 28 pp. 169-199 (1965)