Abstract

We employ an extension of Harrison's theory at the tight binding level of approximation to develop a predictive approach for band gap engineering involving isovalent doping of wide band gap semiconductors. Our results indicate that reasonably accurate predictions can be achieved at qualitative as well as quantitative levels. The predictive results were checked against ab initio ones obtained at the level of DFT/SGGA + U approximation. The minor disagreements between predicted and ab initio results can be attributed to the electronic processes not incorporated in Harrison's theory. These include processes such as the conduction band anticrossing [Shan et al., Phys. Rev. Lett. 82, 1221 (1999); Walukiewicz et al., Phys. Rev. Lett. 85, 1552 (2000)] and valence band anticrossing [Alberi et al., Phys. Rev. B 77, 073202 (2008); Appl. Phys. Lett. 92, 162105 (2008); Appl. Phys. Lett. 91, 051909 (2007); Phys. Rev. B 75, 045203 (2007)], as well as the multiorbital rehybridization. Another cause of disagreement between the results of our predictive approach and the ab initio ones is shown to be the result of the shift of Fermi energy within the impurity band formed at the edge of the valence band maximum due to rehybridization. The validity of our approach is demonstrated with example applications for the systems GaN1− x Sbx , GaP1− x Sbx , AlSb1− x Px , AlP1− xSbx , and InP1− xSbx .

Document Type

Article

Publication Date

3-30-2015

Notes/Citation Information

Published in Journal of Applied Physics, v. 117, no. 12, article 125708, p. 1-9.

Copyright 2015 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.

The following article appeared in Journal of Applied Physics, v. 117, no. 12, article 125708, p. 1-9 and may be found at http://dx.doi.org/10.1063/1.4916252.

Digital Object Identifier (DOI)

http://dx.doi.org/10.1063/1.4916252

Funding Information

M.M. acknowledges funding support from NSF SOLAR project (DMS 1125909) and Kentucky Science and Engineering Foundation (KSEF-13-RDE-017). The support from NSF Award (IIA-1355438) was used to develop the computational techniques.

1.tif (294 kB)
Fig. 1 High-Resolution

Figure 1.pptx (97 kB)
Fig. 1 Powerpoint

2.tif (219 kB)
Fig. 2 High-Resolution

Figure 2.pptx (81 kB)
Fig. 2 Powerpoint

3.tif (132 kB)
Fig. 3 High-Resolution

Figure 3.pptx (60 kB)
Fig. 3 Powerpoint

4.tif (482 kB)
Fig. 4 High-Resolution

Figure 4.pptx (125 kB)
Fig. 4 Powerpoint

5.tif (281 kB)
Fig. 5 High-Resolution

Figure 5.pptx (85 kB)
Fig. 5 Powerpoint

6.tif (1560 kB)
Fig. 6 High-Resolution

Figure 6.pptx (186 kB)
Fig. 6 Powerpoint

7.tif (259 kB)
Fig. 7 High-Resolution

Figure 7.pptx (84 kB)
Fig. 7 Powerpoint

8.tif (263 kB)
Fig. 8 High-Resolution

Figure 8.pptx (84 kB)
Fig. 8 Powerpoint

9.tif (1562 kB)
Fig. 9 High-Resolution

Figure 9.pptx (181 kB)
Fig. 9 Powerpoint

10.tif (245 kB)
Fig. 10 High-Resolution

Figure 10.pptx (89 kB)
Fig. 10 Powerpoint

11.tif (732 kB)
Fig. 11 High-Resolution

Figure 11.pptx (121 kB)
Fig. 11 Powerpoint

Share

COinS