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Journal of Materials Science

, Volume 49, Issue 23, pp 8127–8139 | Cite as

Migration mechanisms of helium in copper and tungsten

  • César GonzálezEmail author
  • Roberto Iglesias
Original Paper

Abstract

A complete set of migration energies for a He atom moving inside the bulk of the bcc-W and fcc-Cu crystals has been calculated in different configurations using the nudged elastic band method as a tool within the density functional theory formalism. Although the most stable site in the perfect crystal is the tetrahedral position in both cases, the He atoms jump preferentially between two first nearest tetrahedral positions in tungsten, while they migrate through an octahedral position in the case of Cu. As reported before, the He atoms are trapped when they find an n-vacancy. Our results show that the migration energies are lower when the n-vacancies do not contain He atoms, suggesting that vacancies are stabilized and their mobility is reduced by helium trapping, that may end up in bubble coalescence, in agreement with previous findings. The migration energy of the clean n-vacancy decreases as the number n increases, at least up to n = 3, while the situation when He atoms are inside the vacancies is a little bit more complicated. In all the analyzed cases, the energy barriers in W are higher than in Cu. Additionally, a complete analysis of the evolution of the electronic density of states has been performed, that leads to the confirmation of a non-negligible He–metal interaction that significantly contributes to the trapping of helium atoms inside the n-vacancies.

Keywords

Fermi Level Energy Barrier Octahedral Site Migration Process Migration Energy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgement

This work has been supported by the FP7 project RADINTERFACES and the Spanish Ministry of Economy and Competitiveness project NANO-EXTREM, Ref. MAT2012-38541. Angel Gutiérrez at the UNIOVI Scientific Modelling Cluster is gratefully acknowledged for technical help and CPU time. Some calculations have been performed thanks to the support provided by the Spanish Supercomputing Network (RES) through the Project FI-2014-1-0008.

Supplementary material

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Supplementary material 1 (MPG 504 kb)
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Copyright information

© Springer Science+Business Media New York 2014

Authors and Affiliations

  1. 1.Departamento de FísicaUniversidad de OviedoOviedoSpain

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