Starting from a quantum mechanical diagrammatic expansion of the grand partition function ξ, and of the coefficients Vbl in the activity expansion of ξ, and making a term by term passage to the limit of classical nuclear motion, results in a corresponding diagrammatic expansion of the Ursell functions Ul(R1, . . ., Rl). Presently only the expansion of the Ursell‐Mayer function f(R) has been explicitly examined and the terms up to second order perturbation theory, including exchange, have been evaluated. The truncated expansion gives a reasonably accurate expression of f(R) for long and medium range distances (R≥4a0) and within this range can be transformed, to the same order of accuracy, into the classical standard form f(R)=exp[ −u(R)]− 1, although in principle an exact formulation in such a form is not necessarily possible.

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See, e.g., G. E. Uhlenbeck and G. W. Ford, Studies in Statistical Mechanics (North‐Holland, Amsterdam, 1962), Vol. 1, Pt. B.
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See, e.g., H. Margenau and N. R. Kestner, Theory of Intermolecular Forces (Pergamon, New York, 1969).
6.
Throughout atomic units (a.u.) are used to represent numerical results. Thus the unit of length is a0 = Bohr radius = 0.53 Å and the unit of energy is e2/a0 = 2Ry = 27.21 eV. The reciprocal temperature β is then given in reciprocal energy atomic units (a.u.−1) so that β = 102a.u.−1 say, is equivalent to T∼3000 °K.
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