Abstract

In 1989, one author of this paper (A.R.) published the very first review paper on InAsSb infrared detectors. During the last thirty years, many scientific breakthroughs and technological advances for InAsSb-based photodetectors have been made. Progress in advanced epitaxial methods contributed considerably to the InAsSb improvement. Current efforts are directed towards the photodetector’s cut-off wavelength extension beyond lattice-available and lattice-strained binary substrates. It is suspected that further improvement of metamorphic buffers for epitaxial layers will lead to lower-cost InAsSb-based focal plane arrays on large-area alternative substrates like GaAs and silicon. Most photodetector reports in the last decade are devoted to the heterostructure and barrier architectures operating in high operating temperature conditions. In the paper, at first InAsSb growth methods are briefly described. Next, the fundamental material properties are reviewed, stressing electrical and optical aspects limiting the photodetector performance. The last part of the paper highlights new ideas in design of InAsSb-based bulk and superlattice infrared detectors and focal plane arrays. Their performance is compared with the state-of-the-art infrared detector technologies.

Highlights

  • The development of InAs1−xSbx (InAsSb) has a long history

  • The III–V semiconductors are characterized by much stronger chemical bonds and higher chemical stability compared to HgCdTe, which is important from the producibility viewpoint

  • Initial reports based on experimental data at temperatures above or near 100 K estimate the direct-gap bowing parameter in InAsSb at 0.58–0.6 eV [50]

Read more

Summary

Introduction

The development of InAs1−xSbx (InAsSb) has a long history. InAsSb was first synthesized in 1958 by Woolley and Smith [1]. Among them we can distinguish IV–VI (Pb1−xSnxTe), and II–VI (Hg1−xCdxTe) infrared (IR) material systems The bandgap of these semiconductors and the spectral response of the devices can be tuned for specific detectors’ applications. Due to large TCE, the indium bonds between silicon readout and the detector array in hybrid structure are exposed to adverse stresses during repeated cooling cycles from room temperature to cryogenic temperature Today this drawback is omitted by fabrication of monolithic PbS and PbSe polycrystalline arrays on Si substrates. The larger valence band energy differences between InAs and GaSb than that between InSb and InAsSb directed mainstream research towards InAs/GaInSb type-II superlattices (T2SLs) allowing larger absorption in LWIR spectral range. This evaluation is supported by theoretical estimates and experimental data

Brief View on Crystal Growth of InAsSb-Based Materials
InAsSb Alloy Properties
Energy Gap
17.9 InSb Bulk BtB
GaAs InP
E Cbaonndduction
Other Properties
77 K 300 K
Bandgap Energy and Effective Masses
Background
Performance Limits
Superlattice Detector Structures
Photodiodes
60 K 70 K 77 K
30 K 40 K
Barrier Detectors
B B Unipolar hole barrier Unipolar hole barrier
77 K 17070 KK 10205 K 112550 KK 115705 KK 127050 KK 220205 KK 225 K
10-6 Background photocurrent
10-6 Red channel
11 ΦΦB ddΦΦB ddTT
Conclusions
Findings
Limitations
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.