Large-scale dynamic Monte Carlo simulations of a lattice gas on a 2000x2000
square lattice with a Glauber-type spin flip dynamics were performed. The
results are discussed in the light of classical nucleation theory (CNT) whi
ch can be fully specified for the problem due to the availability of exact
values for the interfacial energy of a large nucleus, known from the Onsage
r solution. Several alternative (field-theoretic or nonclassical) descripti
ons were also considered. Special attention was paid to the pre-exponential
in the cluster distribution function and to the finite-size corrections to
the interfacial energies which are required in order to comply with observ
ations. If taken literally, the CNT produces large errors when predicting e
ither the cluster distribution function or the nucleation rate. However, at
intermediate temperatures (up to 0.7 T-c) the correspondence can be substa
ntially improved by considering the low-temperature properties of small clu
sters and adjusting the pre-exponential. At higher temperatures the CNT is
in qualitative disagreement with the simulations. Several explanations for
this, including coagulation between clusters, are proposed. (C) 1999 Americ
an Institute of Physics. [S0021-9606(99)51638-3].