We have performed long time scale tight-binding molecular dynamics (MD) sim
ulations to study dimer flippings on perfect and defective Si(0 0 1) surfac
es. The constant temperature MD simulations have been performed for tempera
tures ranging from 800 to 1300 K. From them we measured the average residen
ce time between flips and assuming an Arrhenius equation we obtain a dynami
cal energy barrier for flipping. Our results extrapolate to a dimer flippin
g frequency of 3 x 10(6) Hz at 300 K in agreement with the symmetric appear
ance of surface dimers using STM. We have found that the correlated flippin
gs of two neighbouring dimers are as important as single dimer flippings. T
he ratio of correlated flips with respect to the total number of flips is o
f the order of 0.3 at 800 K and decreases to 0.2 at 1200 K. In the case of
surfaces with a single dimer vacancy, the neighbouring dimers to the vacanc
y have three stable positions instead of two as in perfect surfaces. The di
mers on the same row as the defect flip faster than those of the other row,
leading to their appearance as symmetric dimers in STM measurements at tem
peratures even below the order-disorder transition temperature. (C) 2001 El
sevier Science B.V. All rights reserved.