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First-principles study on composition-dependent properties of quaternary InP1-x-yNxBiy alloys

机译:季型INP1-X-YNXBIY合金组成依赖性的第一原理研究

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The content of bismuth and nitrogen can strongly affect the physical properties of III-V semiconductors and have a decisive impact on their performance in applications. Using first-principles calculations, we systematically study the geometry, electronic and optical properties of InP1-x-yNxBiy aligned in special quasirandom structures (SQS). The incorporation of a small amount of N and Bi can effectively tune the band gap of pristine InP. For the same number of P atoms being substituted, co-doping mode reduced the bond length disparity and the corresponding formation energy was also smaller than that of only nitrogen doped. Since the bismuth doped increases spin-orbit splitting energy (Delta(SO)), the Auger recombination and intervalence band absorption (IVBA) processes are found to be suppressed for quaternary InP0.889N0.037Bi0.074(4.40 mu m), InP0.81.5N0.074Bi0.074 (12.04 mu m) and InP0.815N0.111Bi0.037 (9.12 mu m) alloys, which provides new feasibility in the future mid-wavelength infrared and long-wavelength infrared (MWIR/LWIR) device applications.
机译:铋和氮的含量能够强烈影响III-V半导体的物理性质,并对它们在应用中的性能具有决定性的影响。使用第一原理计算,我们系统地研究了在特殊的Quasirandom结构(SQS)中对齐的INP1-X-YNXBIY的几何形状,电子和光学性质。少量N和BI的掺入可以有效地调整原始INP的带隙。对于所取代的相同数量的P原子,共掺杂模式降低了粘合长度视差,并且相应的形成能量也小于仅掺杂的氮气。由于掺杂的铋增加了旋转轨道分裂能量(Delta(So)),发现螺旋钻重组和逆向带吸收(IVBA)方法被抑制为季型INP0.889N0.037BI0.074(4.40μm),INP0。 81.5N0.074BI0.074(12.04μm)和INP0.815N0.111BI0.037(9.12μm)合金,在未来的中波长红外和长波长红外(MWIR / LWIR)设备应用中提供了新的可行性。

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