The kinetic and potential energies and the pressure of solid neon at room t
emperature have been calculated by means of path-integral Monte Carlo simul
ations using the HFD-C2 pair potential. At these high densities, the quantu
m corrections to the kinetic energy are appreciable, but for the potential
energy and pressure classical simulations (even with a nearest-neighbor mod
el) are generally within 1 % of the quantum-mechanical values. The present
results for the pressure are significantly higher than the experimental equ
ation of state in the 10-100-GPa range. It is shown that inclusion of many-
body short-range interactions might bring the simulations in agreement with
experiment.