Tuning the probability of defect formation via substrate strains in Sr2FeMoO6 films

Waheed A. Adeagbo, Martin Hoffmann, Arthur Ernst, Wolfram Hergert, Minnamari Saloaro, Petriina Paturi, and Kalevi Kokko
Phys. Rev. Materials 2, 083604 – Published 10 August 2018
PDFHTMLExport Citation

Abstract

Since oxide materials like Sr2FeMoO6 are usually applied as thin films, we studied the effect of biaxial strain, resulting from the substrate, on the electronic and magnetic properties and, in particular, on the formation energy of point defects. From our first-principles calculations, we determined that the probability of forming point defects, like vacancies or substitutions, in Sr2FeMoO6 could be adjusted by choosing a proper substrate. For example, the amount of antisite disorder can be reduced with compressive strain in order to obtain purer Sr2FeMoO6 as needed for spintronic applications, while the formation of oxygen vacancies is more likely for tensile strain, which improves the functionality of Sr2FeMoO6 as a basis material of solid oxide fuel cells. In addition, we were also able to include the oxygen partial pressure in our study by using its thermodynamic connection with the chemical potential. Strontium vacancies become, for example, more likely than oxygen vacancies at a pressure of 1bar. Hence, this degree of freedom might offer in general another potential method for defect engineering in oxides aside from, e.g., experimental growth conditions like temperature or gas pressure.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Received 14 May 2018
  • Revised 3 July 2018

DOI:https://doi.org/10.1103/PhysRevMaterials.2.083604

©2018 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Waheed A. Adeagbo1,*, Martin Hoffmann2,†, Arthur Ernst2,3, Wolfram Hergert1, Minnamari Saloaro4, Petriina Paturi4, and Kalevi Kokko5,6

  • 1Institute of Physics, Martin Luther University Halle-Wittenberg, Von-Seckendorff-Platz 1, 06120 Halle, Germany
  • 2Institute for Theoretical Physics, Johannes Kepler University Linz, Altenberger Straße 69, 4040 Linz, Austria
  • 3Max Planck Institute of Microstructure Physics, Weinberg 2, 06120 Halle, Germany
  • 4Wihuri Physical Laboratory, Department of Physics and Astronomy, University of Turku, FI-20014 Turku, Finland
  • 5Department of Physics and Astronomy, University of Turku, FIN-20014 Turku, Finland
  • 6Turku University Centre for Materials and Surfaces (MatSurf), Turku, Finland

  • *waheed.adeagbo@physik.uni-halle.de
  • martin.hoffmann@jku.at

Article Text (Subscription Required)

Click to Expand

Supplemental Material (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 2, Iss. 8 — August 2018

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review Materials

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×