Highly strained In_xGa_(1-x)As-In_yAl _(1-y)As (x>0.8,y<0.3) layers for short wavelength QWIP and QCL structures grown by MBE

Missous, M., Mitchell, C., Sly, J., Lai, K. T., Gupta, R. and Haywood, S. K. (2003) Highly strained In_xGa_(1-x)As-In_yAl _(1-y)As (x>0.8,y<0.3) layers for short wavelength QWIP and QCL structures grown by MBE. Proceedings of the 11th International Conference on Narrow Gap, , Buffalo, NY., United States. 16 - 20 Jun 2003. pp. 496-502 . (doi:10.1016/j.physe.2003.08.066).

Abstract

Highly strained quantum cascade laser (QCL) and quantum well infrared photodetector (QWIPs) structures based on In_xGa _(1-x)As-In_yAl_(1-y)As(x > 0.8,y < 0.3) layers have been grown by molecular beam epitaxy. Conditions of exact stoichiometric growth were used at a temperature of ∼420°C to produce structures that are suitable for both emission and detection in the 2-5 μm mid-infrared regime. High structural integrity, as assessed by double crystal X-ray diffraction, room temperature photoluminescence and electrical characteristics were observed. Strong room temperature intersubband absorption in highly tensile strained and strain-compensated In_0.84Ga _0.16As/AlAs/In_0.52Al_0.48As double barrier quantum wells grown on InP substrates is demonstrated. Γ-Γ intersubband transitions have been observed across a wide range of the mid-infrared spectrum (2-7 μm) in three structures of differing In _0.84Ga_0.16As well width (30, 45, and 80 Å). We demonstrate short-wavelength IR, intersubband operation in both detection and emission for application in QC and QWIP structures. By pushing the InGaAs-InAlAs system to its ultimate limit, we have obtained the highest band offsets that are theoretically possible in this system both for the Γ-Γ bands and the Γ-X bands, thereby opening up the way for both high power and high efficiency coupled with short-wavelength operation at room temperature. The versatility of this material system and technique in covering a wide range of the infrared spectrum is thus demonstrated.

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Contributors

Author: C. Mitchell

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