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We calculate the ground-state energies and pressures for ⁴He and (normal) ³He using radial distribution functions which are solutions of the Born-Bogoliubov-Green-Kirkwood-Yvon (BBGKY) integral equation with the Kirkwood superposition approximation (KSA) used for the three-particle distribution function. We compare the BBGKY-KSA results with those obtained from the hypernetted chain equation, molecular dynamics, and experiment. We conclude that the BBGKY-KSA yields poor results for ⁴He but at the lower ³He densities offers a reasonable approximation to the molecular-dynamics results. The ³He energies are obtained by means of the statistical cluster expansion of Wu and Feenberg and we discuss the convergence of the series. Further, we show that the familiar parametrized power-law form used for the pair function yields pressures consistent with the virial theorem.
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Michael David Miller (1976) studied this question.
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