Published December 1, 2007 | Version v1
Journal article

Simulation of the interaction between Fe impurities and point defects in V

  • 1. Department of Physics, Yeshiva University, New York, New York 10033 (United States)
  • 2. School of Physics, University of Edinburgh, Edinburgh EH9 3JZ, Scotland (United Kingdom)
  • 3. School of Chemistry, Seoul National University, Seoul 151-742 (Korea, Republic of)
  • 4. Department of Physics, Ewha Womans University, Seoul 120-750 (Korea, Republic of)
  • 5. Materials and Engineering Physics, Ames Laboratory, Ames, Iowa 50011 (United States)

Description

We report improved results of atomistic modeling of V-Fe alloys. We introduced an electronic structure embedding approach to improve the description of the point defects in first-principles calculations, by including the semicore electrons in some V atoms (those near the interstitial where the semicore levels are broadened) but not those further from the point defect. This enables us to combine good accuracy for the defect within large supercells and to expand the data set of first-principles point defect calculations in vanadium with and without small amounts of iron. Based on these data, previous first-principles work, and new calculations on the alloy liquid, we fitted an interatomic potential for the V-Fe system which describes the important configurations likely to arise when such alloys are exposed to radiation. This potential is in a form suitable for molecular dynamics (MD) simulations of large systems. Using the potential, we have calculated the migration barriers of vacancies in the presence of iron, showing that these are broadly similar. On the other hand, MD simulations show that V self-diffusion at high temperatures and Fe diffusion are greatly enhanced by the presence of interstitials

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. B, Condensed Matter and Materials Physics
Journal Volume
76
Journal Issue
21
Journal Page Range
p. 214105-214105.11
ISSN
1098-0121

Optional Information

Notes
(c) 2007 The American Physical Society