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ithe Ornstein-Zernike relation was used to Calculate the pair distribution runc- tion, g(1, 2), from our direct correlation function data. Outside the overlap region, the agreement with simulation results is excellent, even for hard spheres close to freezing. Within the overlap region,however, the pair distribution function is not zero as it should be. For spheres, adding more terms in the virial expansion pro- gressively reduces this discrepancy and at 6" order, the core condition is fairly well obeyed. For spheroids, one must consider both the truncation of the virial series and also the truncation of the angular expansion of c(1, 2) in spherical harmonics. We believe that the violation of the core condition is associated with both these truncations and, in a future publication, we will present a systematic study of the effects of including higher order angular terms.

Figure 6 ithe Ornstein-Zernike relation was used to Calculate the pair distribution runc- tion, g(1, 2), from our direct correlation function data. Outside the overlap region, the agreement with simulation results is excellent, even for hard spheres close to freezing. Within the overlap region,however, the pair distribution function is not zero as it should be. For spheres, adding more terms in the virial expansion pro- gressively reduces this discrepancy and at 6" order, the core condition is fairly well obeyed. For spheroids, one must consider both the truncation of the virial series and also the truncation of the angular expansion of c(1, 2) in spherical harmonics. We believe that the violation of the core condition is associated with both these truncations and, in a future publication, we will present a systematic study of the effects of including higher order angular terms.