Study of the valence band offsets between InAs and InAs 1-x Sb x alloys

Elizabeth H. Steenbergen, O. O. Cellek, D. Lubyshev, Yueming Qiu, J. M. Fastenau, Amy W. K. Liu, Yong‐Hang Zhang

Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · 2011 · 15 citations · 0 references

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Abstract

InAs/InAs<sub>1-x</sub>Sb<sub>x</sub> strain-balanced superlattices (SLs) on GaSb are a viable alternative to the well-studied InAs/Ga<sub>1-x</sub>In<sub>x</sub>Sb SLs for mid- and long-wavelength infrared (MWIR and LWIR) laser and photodetector applications, but the InAs/InAs<sub>1-x</sub>Sb<sub>x</sub> SLs are not as thoroughly investigated. Therefore, the valence band offset between InAs and InAs/InAs<sub>1-x</sub>Sb<sub>x</sub>, a critical parameter necessary to predict the SL bandgap, must be further examined to produce InAs/InAs<sub>1-x</sub>Sb<sub>x</sub> SLs for devices operational at MWIR and LWIR wavelengths. The effective bandgap energies of InAs/InAs<sub>1-x</sub>Sb<sub>x</sub> SLs with x = 0.28 - 0.40 are designed using a three-band envelope function approximation model. Multiple 0.5 &#956;m-thick SL samples are grown by molecular beam epitaxy on GaSb substrates. Structural characterization using x-ray diffraction and atomic force microscopy reveals excellent crystalline properties with SL zero-order peak full-width-half-maximums between 30 and 40 arcsec and 20 x 20 &#956;m2 area root-mean-square roughnesses of 1.6 - 2.7 A. Photoluminescence (PL) spectra of these samples cover 5 to 8 &#956;m, and the band offset between InAs and InAs/InAs<sub>1-x</sub>Sb<sub>x</sub> is obtained by fitting the PL peaks to the calculated values. The bowing in the valence band is found to depend on the initial InAs/InSb valence band offset and changes linearly with x as C<sub>Ev_bowing </sub>= 1.58x - 0.62 eV when an InAs/InAs<sub>1-x</sub>Sb<sub>x</sub> bandgap bowing parameter of 0.67 eV is assumed. A fractional valence band offset, Q<sub>v</sub> = &#916;E<sub>v</sub>/&#916;E<sub>g</sub>, of 1.75 ± 0.03 is determined and is practically constant in the composition range studied.