2020
DOI: 10.1063/5.0007512
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Strain dependence of Auger recombination in 3 μm GaInAsSb/GaSb type-I active regions

Abstract: We differentiate the effect of strain induced by lattice-mismatched growth from strain induced by mechanical deformation on cubic nonradiative Auger recombination in narrow-gap GaInAsSb/GaSb quantum well (QW) heterostructures. The typical reduction in the Auger coefficient observed with lattice-mismatched growth appears to be due to the concomitant compositional change rather than the addition of strain, with implications for mid-IR semiconductor laser design. We induced a range of internal compressive strain … Show more

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Cited by 3 publications
(9 citation statements)
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“…Figure 4 expands that analysis by including the converted 3D results for T1QWs (red points) [16], [17], [19], [29]- [30], [33]- [40]. The open red points are extracted from threshold data acquired at University of Surrey using hydrostatic pressure to vary the bandgap, and hence the emission wavelength, of a given device [19].…”
Section: "3d" Auger Coefficientsmentioning
confidence: 89%
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“…Figure 4 expands that analysis by including the converted 3D results for T1QWs (red points) [16], [17], [19], [29]- [30], [33]- [40]. The open red points are extracted from threshold data acquired at University of Surrey using hydrostatic pressure to vary the bandgap, and hence the emission wavelength, of a given device [19].…”
Section: "3d" Auger Coefficientsmentioning
confidence: 89%
“…This supposition was supported by the measurement of a relatively high Auger coefficient for a type-I InAs0.85Sb0.15-In0.87Al0.13As0.91Sb0.09 multiple quantum well (MQW) [28]. However, several groups subsequently showed that mid-IR InGa(As)Sb T1QWs, with GaSb or AlGa(In)AsSb barriers and grown on GaSb with much greater strain, can also display significant suppression of the Auger decay rate [13], [16], [17], [19]. This is not really surprising since, as in T2QWs, compressive strain splits the valence band degeneracy at k = 0 and induces a much lighter in-plane heavy hole mass near the zone center.…”
Section: Figurementioning
confidence: 97%
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