As part of our investigations on the disordering of metal surfaces, we
report the results of our calculations of the energetics of formation
and migration of defects in Pb(110) using molecular-dynamics and mole
cular-statics simulations. We used the embedded-atom method to describ
e the interatomic interactions. Defect formation and migration energie
s have been calculated at the surface as well as in the near-surface r
egion. Vacancy, divacancy, and interstitial formation and migration en
ergies converge to bulk values already at a few layers below the surfa
ce. Our results are compared with recent simulations of Cu and Ni and
with experimental data. We also calculated the surface Debye temperatu
re and surface energy. We find that the surface Debye temperature, sur
face single-vacancy formation energy, and surface divacancy formation
energy are all lower than their bulk values. Our result for the surfac
e energy is lower than the experimental values.