Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-25T01:53:45.880Z Has data issue: false hasContentIssue false

Magnetic Properties of Polar ZnO Surfaces from Ab-initio Calculations

Published online by Cambridge University Press:  23 June 2011

Guntram Fischer
Affiliation:
Institut für Physik, Martin-Luther-Universität Halle-Wittenberg, Von-Seckendorff-Platz 1, 06120 Halle, Germany
Nadiezhda Sanchez
Affiliation:
Instituto de Ciencia de Materiales de Madrid, 28049 Madrid, Spain
Waheed A. Adeagbo
Affiliation:
Institut für Physik, Martin-Luther-Universität Halle-Wittenberg, Von-Seckendorff-Platz 1, 06120 Halle, Germany
Martin Lüders
Affiliation:
Daresbury Laboratory, Daresbury, Warrington, WA4 4AD, U.K.
Zdzislawa Szotek
Affiliation:
Daresbury Laboratory, Daresbury, Warrington, WA4 4AD, U.K.
Walter Temmerman
Affiliation:
Daresbury Laboratory, Daresbury, Warrington, WA4 4AD, U.K.
Arthur Ernst
Affiliation:
Max-Planck-Institut für Mikrostrukturphysik, Weinberg 2, 06120 Halle, Germany
Wolfram Hergert
Affiliation:
Institut für Physik, Martin-Luther-Universität Halle-Wittenberg, Von-Seckendorff-Platz 1, 06120 Halle, Germany
M. Carmen Muñoz
Affiliation:
Instituto de Ciencia de Materiales de Madrid, 28049 Madrid, Spain
Get access

Abstract

We have studied the effect that applying self-interaction correction (SIC) to oxygen p orbitals has on the magnetic moment formation of three polar ZnO surfaces; all of them being oxygen terminated. For these investigations we have used a multi-code approach. This has allowed us, on the one hand, to relax the surface structure using the pseudopotential code SIESTA. On the other hand, by using the obtained relaxed structures for calculations within the KKR Green’s function formalism, we have been able to apply SIC and use the magnetic force theorem for calculating Heisenberg exchange parameters. The latter contain information about both the strength of the interaction and the interaction mechanism.

Our calculations show that all three surfaces are magnetic. In addition, we find that applying SIC is necessary to correctly describe the top oxygen atom of the (0001)-t and (0001)-h surfaces.

Type
Research Article
Copyright
Copyright © Materials Research Society 2011

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

1. Zunger, A., Lany, S. and Raebiger, H., Physics 3, 53 (2010).Google Scholar
2. Droghetti, A., Pemmaraju, C. D. and Sanvito, D., Phys. Rev. B 78, 140404 (2008).Google Scholar
3. Adeagbo, W. A., Fischer, G., Ernst, A. and Hergert, W., J. Phys.: Condens. Matter 22, 436202 (2010).Google Scholar
4. Khalid, M., Ziese, M., Setzer, A. et al. ., Phys. Rev. B 80, 035331 (2009).Google Scholar
5. Stoneham, M., J. Phys.: Condens. Matter 22, 074211 (2010).Google Scholar
6. Khalid, M., Setzer, A., Ziese, M., Esquinazi, P., Spemann, D., Pöppl, A. and Goering, E., Phys. Rev. B 81, 214414 (2010).Google Scholar
7. Straumal, B. B., Mazilkin, A. A., Protasova, S. G., Myatiev, A. A., Straumal, P. B., Schütz, G., van Aken, P. A., Goering, E. and Baretzky, B., Phys. Rev. B 79, 205206 (2009).Google Scholar
8. Gallego, S., Beltrán, J. I., Cerdá, J., and Muñoz, M. C., J. Phys: Condens. Matter 17, L451 (2005).Google Scholar
9. Sanchez, N., Gallego, S. and Muñoz, M. C., Phys. Rev. Lett. 101, 067206 (2008).Google Scholar
10. Soler, J. M., Artacho, E., Gale, J. D., García, A., Junquera, J., Ordejón, P. and Sánchez-Portal, D., J. Phys.: Condens. Matter 14, 2745 (2002).Google Scholar
11. Lüders, M., Ernst, A., Däne, M., Szotek, Z., Svane, A., Ködderitzsch, D., Hergert, W., Gyorffy, B. L. and Temmerman, W. M., Phys. Rev. B 71, 205109 (2005).Google Scholar
12. Liechtenstein, A., Katsnelson, M., Antropov, V. and Gubanov, V., J. of Mag. Mag. Mat. 67, 65 (1987).Google Scholar
13. Şaşıoğlu, E., Sandratskii, L. M., Bruno, P. and Galanakis, I., Phys. Rev. B 72, 184415 (2005).Google Scholar
14. Kresse, G., Dulub, O. and Diebold, U., Phys. Rev. B 68, 245409 (2003).Google Scholar