“…In InAs binary alloy, it forms as the antibonding A 1 state and is about 30 meV below the conduction band edge of InAs which holds the same position in strain. This state is within 4 meV of the reported SRH recombination The Sb A s antisites related to the Sb diffusion at the SL interfaces could cause localized defect states, however, the energy level of these antisites is more than an eV below the InAs valence band edge[97].4.3.2.2 Radiative RecombinationThe calculated radiative coefficients are in range of 1.5 − 3× 10 −10 cm 3 /s for the samples with 30 % and 40 % Sb content in their alloy layers at 77 K. These coefficients gradually decrease to 2 − 5× 10 −11 cm 3 /s at 200 K. The radiative recombination coefficients of all the InAs/InAsSb T2SLs examined in this sample set, were found to be essentially insignificant at high excess carrier densities for the temperatures ranging[49], low surface leakage[98], and high material quality[13], they unfortunately suffer from relatively high Auger recombination rates[9,22,45]. For materials that are not limited by Shockley-Read-Hall (SRH) recombination, intrinsic Auger recombination rates typically define a photodetectors maximum attainable carrier lifetime and, hence best case dark diffusion current[99].…”