GaSb1-xBix layers with 0 < x ≤ 0.042 have been studied by photoreflectance in 15-290 K temperature range. We found that due to the incorporation of Bi atoms into the GaSb host, the E0 band gap-related transition redshifts (∼30 meV per 1% Bi) and significantly broadens. The shift of the E0 transition in the temperature range 10-270 K has been found to be ∼70 meV, very similar to the energy shift in GaSb over the same temperature range. We analyzed the energy and broadening of the E0 transition using the Varshni and Bose-Einstein formulas and found that the Varshni and Bose-Einstein parameters of GaSb1-xBi x are similar to those of GaSb. Moreover we concluded that the inhomogeneities in GaSb1-xBix alloys is less important than in dilute bismide arsenides since Bi atoms are more similar to Sb atoms (in electronegativities and ionic sizes). © 2013 AIP Publishing LLC.
CITATION STYLE
Kopaczek, J., Kudrawiec, R., Linhart, W. M., Rajpalke, M. K., Yu, K. M., Jones, T. S., … Veal, T. D. (2013). Temperature dependence of the band gap of GaSb1-xBix alloys with 0 < x ≤ 0.042 determined by photoreflectance. Applied Physics Letters, 103(26). https://doi.org/10.1063/1.4858967
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