Abstract
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.
| Original language | English |
|---|---|
| Article number | 261907 |
| Journal | Applied Physics Letters |
| Volume | 103 |
| Issue number | 26 |
| DOIs | |
| Publication status | Published - 23 Dec 2013 |
| Externally published | Yes |
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