Abstract
Transitions between “glassy” local minima of a model free-energy functional for a dense hard-sphere system are studied numerically using a “microcanonical” Monte Carlo method that enables us to obtain the transition probability as a function of the free energy and the Monte Carlo “time.” The growth of the height of the effective free-energy barrier with density is found to be consistent with a Vogel-Fulcher law. The dependence of the transition probability on time indicates that this growth is primarily due to an increase in the difficulty of finding low-free-energy paths to other minima.
Original language | English (US) |
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Pages (from-to) | 801-804 |
Number of pages | 4 |
Journal | Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics |
Volume | 58 |
Issue number | 1 |
DOIs | |
State | Published - 1998 |