Properties of the free-energy landscape in phase space of a dense hard-sphe
re system characterized by a discretized free-energy functional of the Rama
krishnan-Yussouff form are investigated numerically. A considerable number
of glassy local minima of the free energy are located and the distribution
of an appropriately defined 'overlap' between minima is calculated. The pro
cess of transition from the basin of attraction of a minimum to that of ano
ther one is studied using a new 'microcanonical' Monte Carlo procedure, lea
ding to a determination of the effective height of free-energy barriers tha
t separate different glassy minima. The general appearance of the free-ener
gy landscape resembles that of a putting green: deep minima separated by a
fairly Rat structure. The growth of the effective free-energy barriers with
increasing density is consistent with the Vogel-Fulcher law, and this grow
th is primarily driven by an entropic mechanism.