Abstract

Both the formation energies, the intra-layer and inter-layer diffuse migration energies of a single vacancy in the first nine layers of the Fe (1 1 0) surface have been calculated by means of molecular dynamics in conjunction with the many-body potential of the embedded-atom method (EAM). The results show that the effect of the surface is only down to the fourth layer for the formation energy of a single vacancy. However, the surface presence affects the migration energy down to the seventh layer. It is easier for a vacancy in the first layer to form and to migrate than in the other layers and the bulk. For the inter-layer migration, a vacancy in each of the first six layers is favorable to migrate into the corresponding upper layer, especially for the first three layers.

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call