NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
InAsSbBi, a direct band-gap, III-V, LWIR materialIn the last several years Dr. Stringfellow's group at the University of Utah has reported success in incorporating over 3 percent Bi in InAs and 1.5 percent in InAsSb using Organometallic Vapor Phase Epitaxy (OMVPE) growth techniques. For InAs the lattice constant increase is linear with a=6.058+0.966x (InAs(1-x)Bi(x)), and a decrease in band gap energy of dEg / dx = -55meV / at a percentage Bi. Extrapolating this to the ternary minimum band gap at InAs(0.35)Sb(0.65), an addition of 1 to 2 percent Bi should drop the band gap to the 0.1 to 0.05eV range (10 to 20 microns). These alloys are direct band gap semiconductors making them candidates for far IR detectors. The current status of the InAsSbBi alloys is that good crystal morphology and x ray diffraction data has been obtained for up to 3.4 percent Bi. The Bi is metastable at these concentrations but the OMVPE grown material has been able to withstand the 400 C growth temperature for several hours without phase separation.
Document ID
19910005097
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Stringfellow, G. B.
(Utah Univ. Salt Lake City., United States)
Jones, Colin E.
(Santa Barbara Focalplane Goleta, CA., United States)
Frodsham, John
(Space Systems Engineering Logan, UT., United States)
Date Acquired
September 6, 2013
Publication Date
July 1, 1990
Publication Information
Publication: JPL, California Inst. of Tech., Innovative Long Wavelength Infrared Detector Workshop Proceedings
Subject Category
Spacecraft Instrumentation
Accession Number
91N14410
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available