Published February 1, 2010 | Version v1
Journal article

Migration of Cr-vacancy clusters and interstitial Cr in α-Fe using the dimer method

  • 1. Pacific Northwest National Laboratory, P.O. Box 999, Richland, Washington 99352 (United States)
  • 2. Department of Applied Physics, Hunan University, Changsha 410082 (China)
  • 3. SCK-CEN, Nuclear Science Institute, Boeretang 200, B-2400 Mol (Belgium)

Description

The migration mechanisms and the corresponding activation energies of Cr-vacancy (Cr-V) clusters and Cr interstitials in α-Fe have been investigated using the dimer and the nudged elastic-band methods. Dimer searches are employed to find the possible transition states of these defects and the lowest-energy paths are used to determine the energy barriers for migration. A substitutional Cr atom can migrate to a nearest-neighbor vacancy through an energy barrier of 0.56 eV but this simple mechanism alone is unlikely to lead to the long-distance migration of Cr unless there is a supersaturated concentration of vacancies in the system. The Cr-vacancy clusters can lead to long-distance migration of a Cr atom that is accomplished by Fe and Cr atoms successively jumping to nearest-neighbor vacancy positions, defined as a self-vacancy-assisted migration mechanism, with the migration energies ranging from 0.64 to 0.89 eV. In addition, a mixed Cr-Fe dumbbell interstitial can easily migrate through Fe lattices, with the migration energy barrier of 0.17, which is lower than that of the Fe-Fe interstitial. The on-site rotation of the Cr-Fe interstitial and Cr atom hopping from one site to another are believed to comprise the dominant migration mechanism. The calculated binding energies of Cr-V clusters are strongly dependent on the size of clusters and the concentration of Cr atoms in clusters.

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. B, Condensed Matter and Materials Physics
Journal Volume
81
Journal Issue
6
Journal Page Range
p. 064101-064101.9
ISSN
1098-0121

Optional Information

Notes
(c) 2010 The American Physical Society