Interactions between hydrogen impurities and vacancies in Mg and Al: A comparative analysis based on density functional theory

Lars Ismer, Min Sik Park, Anderson Janotti, and Chris G. Van de Walle
Phys. Rev. B 80, 184110 – Published 17 November 2009; Erratum Phys. Rev. B 81, 139902 (2010)

Abstract

Using first-principles methods we have studied the interactions between hydrogen impurities and vacancies in hcp Mg and fcc Al. We find that single vacancies can, in principle, host up to 9 H atoms in Mg and 10 in Al, not 12 as recently reported in the case of Al. The difference between our results and the results in previous work is attributed to a more appropriate definition of the trapping energy of hydrogen impurities in vacancies. The concentration of hydrogen-vacancy complexes depends on the amount of hydrogen dissolved in the metal, which in turn is dictated by the hydrogen chemical potential μH. We evaluated the concentration of all relevant hydrogen-vacancy complexes as a function of μH, corresponding to different H loading conditions—ranging from low pressures to high pressures of H2 gas, up to hydrogen plasma conditions. Our analysis reveals fundamental differences in the characteristics of the hydrogen-vacancy interaction between Mg and Al. In the case of Al, up to 15% of H atoms are trapped in single vacancies in the form of H-vacancy complexes even for very low values of μH. The trapping effect slows down the diffusion of H atoms in Al by more than an order of magnitude. While interactions between vacancies and single hydrogen atoms are therefore clearly important, interactions with multiple H atoms and related mechanisms (such as hydrogen-induced superabundant vacancy formation) are predicted to occur in Al only at very high values of μH. In the case of Mg, the effects of H trapping in single vacancies are negligible for low values of μH due to the relatively low formation energy of isolated interstitial H. However, vacancies containing multiple H atoms and related mechanisms such as hydrogen-induced superabundant vacancy formation are predicted to occur in Mg at much lower values of μH than in Al. We estimate that, at room temperature, the critical pressure of an H2 gas to induce hydrogen-enhanced (superabundant) vacancy formation is 1GPa in Mg and 10GPa in Al.

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  • Received 24 July 2009

DOI:https://doi.org/10.1103/PhysRevB.80.184110

©2009 American Physical Society

Erratum

Authors & Affiliations

Lars Ismer1,2, Min Sik Park1,3, Anderson Janotti1, and Chris G. Van de Walle1

  • 1Materials Department, University of California, Santa Barbara, California 93106-5050, USA
  • 2Abteilung Computergestütztes Materialdesign, Max-Planck-Institut für Eisenforschung GmbH, Max-Planck-Strasse 1, 40237 Düsseldorf, Germany
  • 3Department of Physics, Missouri University of Science and Technology, Rolla, Missouri 65409, USA

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Issue

Vol. 80, Iss. 18 — 1 November 2009

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