Indium gallium arsenide

What Is Indium Gallium Arsenide?

Indium gallium arsenide (InGaAs), with the chemical formula In(x)Ga(1-x)As, is a ternary III-V semiconductor alloy formed by substituting a fraction of gallium atoms in gallium arsenide with indium. By varying the indium mole fraction x between 0 and 1, the material's bandgap shifts continuously from 1.42 eV (pure GaAs) down to 0.36 eV (pure InAs), covering the near-infrared spectral region that includes the low-loss transmission windows of silica optical fiber at 1.3 and 1.55 micrometers. InGaAs draws on semiconductor physics, crystal growth science, and device engineering, and it is among the most widely deployed III-V materials in high-speed electronics and fiber-optic systems.

The composition most commonly encountered in device work is In(0.53)Ga(0.47)As, which is lattice-matched to indium phosphide substrates. This composition yields a bandgap of approximately 0.74 eV and an electron mobility near 10,000 cm2/V-s at room temperature, roughly three to five times higher than silicon under comparable doping conditions. Lattice matching to InP is important because growing a mismatched epitaxial layer introduces dislocations that degrade carrier transport and optical efficiency.

Material Properties and Bandgap Engineering

The tunable bandgap of InGaAs is its defining feature from an engineering standpoint. Adjusting indium content shifts the absorption edge, allowing designers to target specific wavelengths for detection or emission. In photodetector applications, the In(0.53)Ga(0.47)As composition absorbs efficiently at the 1.3 and 1.55 micrometer wavelengths used in long-haul fiber-optic transmission, while compositions with higher indium fractions extend sensitivity further into the mid-infrared. The relationship between composition, lattice parameter, and bandgap for the InGaAs alloy system is well characterized in detailed semiconductor overviews from ScienceDirect, which also document the strained-layer variants used when lattice mismatch is deliberately introduced to enhance particular properties.

The high electron mobility of InGaAs arises from the light effective mass of conduction-band electrons in the alloy. This property drives much of the research into InGaAs metal-oxide-semiconductor field-effect transistors (MOSFETs) as potential successors to silicon at sub-10 nm gate lengths, where silicon's lower mobility imposes fundamental speed limits.

High-Speed Electronics

InGaAs is the active-channel material in high-electron-mobility transistors (HEMTs), which are used extensively in microwave and millimeter-wave amplifiers. In an InGaAs HEMT, the channel lies in a thin InGaAs quantum well sandwiched between wider-bandgap InAlAs barrier layers, and the spatial separation of the channel from its parent donors suppresses impurity scattering, yielding high transconductance and noise figures below 1 dB at tens of gigahertz. These devices underpin low-noise amplifiers in satellite receivers, radio-telescope front ends, and emerging 5G millimeter-wave radios. Research at institutions such as MIT has investigated InGaAs channels as replacements for silicon in CMOS logic, as reported in Semiconductor Today's coverage of IEDM presentations on InGaAs transistors.

Photodetectors and Imaging

The primary optoelectronic application for InGaAs is the photodetector. PIN photodiodes and avalanche photodiodes fabricated in In(0.53)Ga(0.47)As achieve high quantum efficiency across the C-band and L-band of optical fiber systems. InGaAs avalanche photodiodes offer 8 to 10 dB better receiver sensitivity than PIN diode counterparts in digital optical links, as documented in IEEE Xplore publications on InGaAs avalanche photodiodes. Two-dimensional InGaAs focal-plane arrays are deployed in shortwave-infrared cameras used for industrial inspection, night vision, and hyperspectral imaging.

Applications

Indium gallium arsenide has applications in a wide range of fields, including:

  • Fiber-optic receivers and transceivers for telecommunications
  • Low-noise amplifiers in satellite and microwave radio systems
  • Shortwave-infrared cameras for industrial and scientific imaging
  • High-efficiency multijunction solar cells for space power
  • Millimeter-wave and sub-terahertz front-end circuits
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