Hostname: page-component-848d4c4894-xm8r8 Total loading time: 0 Render date: 2024-06-19T04:20:09.308Z Has data issue: false hasContentIssue false

Experimental Evidence for Nitrogen as a Deep Acceptor in ZnO

Published online by Cambridge University Press:  29 December 2011

M.C. Tarun
Affiliation:
Department of Physics and Materials Science Program, Washington State University Pullman, WA 99164-2814, U.S.A.
M. Zafar Iqbal
Affiliation:
Department of Physics, COMSATS Institute of Information Technology Islamabad 44000, Pakistan
M.D. McCluskey
Affiliation:
Department of Physics and Materials Science Program, Washington State University Pullman, WA 99164-2814, U.S.A.
J. Huso
Affiliation:
Department of Physics, University of Idaho Moscow, ID 83844, U.S.A.
L. Bergman
Affiliation:
Department of Physics, University of Idaho Moscow, ID 83844, U.S.A.
Get access

Abstract

While zinc oxide is a promising material for blue and UV solid-state lighting devices, the lack of p-type doping has prevented ZnO from becoming a dominant material for optoelectronic applications. Over the past decade, numerous reports have claimed that nitrogen is a viable p-type dopant in ZnO. However, recent calculations by Lyons, Janotti, and Van de Walle [Appl. Phys. Lett. 95, 252105 (2009)] suggest that nitrogen is a deep acceptor. In our work, we performed photoluminescence (PL) measurements on bulk, single crystal ZnO grown by chemical vapor transport. Nitrogen doping was achieved by growing in ammonia. In prior work at room temperature, we observed a broad PL band at ∼1.7 eV, with an excitation threshold of ∼2.2 eV, consistent with the calculated configuration-coordinate diagram. In the present work, at liquid-helium temperatures, the PL emission increases in intensity and red-shifts by ∼0.2 eV. A peak is observed at 3.267 eV, which we tentatively attribute to an exciton bound to a nitrogen acceptor. Our experimental results indicate that nitrogen is indeed a deep acceptor and cannot be used to produce p-type ZnO.

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. Chen, Y., Bagnall, D.M., Koh, H.-J., Park, K.-T., Hiraga, K., Zhu, Z.-Q., and Yao, T., J. Appl. Phys. 84, 3912 (1998).Google Scholar
2. McCluskey, M.D. and Jokela, S.J., J. Appl. Phys. 106, 071101 (2009).Google Scholar
3. Thonke, K., Gruber, T., Teofilov, N., Schnfelder, R., Waag, A., and Sauer, R., Physica B 308310, 945 (2001).Google Scholar
4. Zeuner, A., Alves, H., Hoffman, D.M., Meyer, B.K., Hoffmann, A., Haboeck, U., Strassburg, M. and Dworzak, M., Phys. Status Solidi B 234, R7 (2002).Google Scholar
5. Wang, L. and Giles, N.C., Appl. Phys. Lett. 84, 3049 (2004).Google Scholar
6. Duan, X.M., Stampfl, C., Bilek, M.M.M., McKenzie, D.R., and Wei, S.-H., Phys. Rev. B 83, 085202.Google Scholar
7. Park, C.H., Zhang, S.B., and Wei, S.-H., Phys. Rev. B 66, 073202 (2002).Google Scholar
8. Bierwagen, O., Ive, T., Van de Walle, C.G., and Speck, J.S., Appl. Phys. Lett. 93, 242108 (2008).Google Scholar
9. Lyons, J.L., Janotti, A., and Van de Walle, C.G., Appl. Phys. Lett. 95, 252105 (2009).Google Scholar
10. Lany, S. and Zunger, A., Phys. Rev. B 81, 205209 (2010).Google Scholar
11. Tarun, M.C., Zafar Iqbal, M., and McCluskey, M.D., AIP Advances 1, 022105 (2011).Google Scholar
12. Haynes, J.R., Phys. Rev. Lett. 4, 361 (1960).Google Scholar
13. Teklemichael, S.T., Hlaing Oo, W.M., McCluskey, M.D., Walter, E.D., and Hoyt, D.W., Appl. Phys. Lett. 98, 232112 (2011).Google Scholar