The temporal evolution and morphology of grain growth in three dimensi
ons were simulated by Monte Carlo method. In order to prevent impingem
ent of grains of like orientation, new algorithm was adopted. The anis
otropy of the grain boundary energy is incorporated into the model. Co
mpared with the case in which no anisotropy of boundary energy is assu
med, the suppression of grain growth was observed at the initial stage
of growth in the grain structure with anisotropic grain boundary ener
gy. However, the growth rate is higher at the later stage. The grain s
ize and the face number distributions become broad. To evaluate the pr
ofile of the grain size distribution, a parameter called microstructur
al entropy, S, is defined. It was shown that the characteristics of si
ze distribution profile may be represented by the value S. The average
size of n-faced grain is proportional to the grain face number, n. Th
e effect of the anisotropy of grain boundary energy on the n-dependenc
e of the average grain size is not evident, The nearest neighbour face
number correlation similar to the Aboav-Weaire relation in two dimens
ion is observed in both grain structures with isotropic grain boundary
energy and anisotropic grain boundary energy.