Small bandgap IR detectors need to work in crogenic temperature

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SUMMARY

Small bandgap infrared (IR) detectors, such as InSb photodetectors, require operation at cryogenic temperatures to minimize thermal noise, which can significantly affect their performance. The thermal energy at room temperature (approximately 0.0259 eV) is sufficient to excite a considerable number of electrons across the 0.17 eV bandgap of InSb, leading to increased noise levels. The discussion highlights that the detectivity of these photodetectors is inversely proportional to the square root of the carrier capture time, suggesting that longer capture times could enable higher temperature operation without compromising sensitivity.

PREREQUISITES
  • Understanding of semiconductor physics, particularly bandgap energy
  • Knowledge of infrared detection technologies, specifically InSb photodetectors
  • Familiarity with thermal noise concepts in electronic systems
  • Basic grasp of carrier dynamics and capture time in semiconductors
NEXT STEPS
  • Research the principles of cryogenic cooling techniques for infrared detectors
  • Explore the relationship between carrier capture time and photodetector performance
  • Study the thermal noise characteristics in semiconductor devices
  • Investigate alternative materials with varying bandgap energies for IR detection
USEFUL FOR

This discussion is beneficial for optical engineers, materials scientists, and researchers involved in the development and optimization of infrared detection systems, particularly in applications requiring high sensitivity and low thermal noise.

chenhon5
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Is anybody can give me a detailed explanation or reference why the small bandgap IR detectors (eg. InSb photodetecotr) need to work in the cryogenic temperature?

In addition, anybody knows what is carrier capture time? Since some article said the photodetector detectivity is proportional to the square root of the carrier capture time, so increased capture time have the potential for higher temperature operation. Any thought? Thanks.
 
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A small band gap means that very little energy is needed to knock an electron out of the band and make it conduct.
At room temperature there is enough thermal energy to do this with a large number of electrons.
It depends on how much sensitivity you need, how strong your signal is compared to the thermal noise, so firefighters infrared displays aren't cooled but astronomical cameras are.
 
mgb_phys said:
A small band gap means that very little energy is needed to knock an electron out of the band and make it conduct.
At room temperature there is enough thermal energy to do this with a large number of electrons.
It depends on how much sensitivity you need, how strong your signal is compared to the thermal noise, so firefighters infrared displays aren't cooled but astronomical cameras are.

Thank you for your reply. As I know the energy due to the temperature is k*T=0.0259eV, however, the bandgap of InSb is about 0.17eV, which is much larger than the thermal noise. Do you mean even the bandgap of InSb is larger than the thermal noise, but their values are more closed than other materials (say 1eV), so they will knock out much more electrons than wide bandgap materials?

Do you have an idea for the second question for my post about the carrier capture time?
 

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