“…The most important effect of the substitutions in these InN x As 1−x , InN x Sb 1−x and InAs x Sb 1−x alloys is large reduction of the fundamental band gap (E Γ g ) of InAs and InSb. In the literature, the aim dependent reduction of the fundamental energy gap has been tuned by the substituent compositions in InNAs, InNSb and InAsSb alloys [8,[11][12][13][14][15][16][17][18][20][21][22][23][24][25][26][27] grown by molecular beam epitaxy (MBE) [12,[14][15][16][17]21,22,24], metal organic chemical vapor deposition (MOCVD) [8,11,13,23,25], Bridgman [26] and hotwall epitaxy (HWE) [28] methods. Therefore, these ternary alloys are potential materials for room temperature infrared detectors, gas sensors and lasers operating in near-infrared (0.9-1.3 m), mid-infrared (2-5 m) and far infrared (8-12 m) regions [13,17,[21][22][23][24][25][26].…”