2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/19365Monte Carlo simulations on the structural properties of ternary fluid mixtures of additive hard spheres are reported. The results are compared with those obtained from a recent analytical approximation [S. B. Yuste, A. Santos, and M. Lopez de Haro, J. Chem. Phys. 108, 3683 (1998)] to the radial distribution functions of hard-sphere mixtures and with the results derived from the solution of the Ornstein-Zernike integral equation with both the Martynov-Sarkisov and the Percus-Yevick closures. Very good agreement between the results of the first two approaches and simulation is observed, with a noticeable improvement over the Percus-Yevick predictions especially near contact.11 pages, including 8 figures; A minor change; accepted for publication in PREStatistical MechanicsSoft Condensed MatterChemical PhysicsStructure of ternary additive hard-sphere fluid mixturestext