Abstract

This work demonstrates a mid-wavelength infrared InAs/InSb superlattice avalanche photodiode (APD). The superlattice APD structure was grown by molecular beam epitaxy on GaSb substrate. The device exhibits a 100 % cut-off wavelength of 4.6 µm at 150 K and 4.30 µm at 77 K. At 150 and 77 K, the device responsivity reaches peak values of 2.49 and 2.32 A/W at 3.75 µm under −1.0 V applied bias, respectively. The device reveals an electron dominated avalanching mechanism with a gain value of 6 at 150 K and 7.4 at 77 K which was observed under −6.5 V bias voltage. The gain value was measured at different temperatures and different diode sizes. The electron and hole impact ionization coefficients were calculated and compared to give a better prospect of the performance of the device.

Highlights

  • Detectors with a capability of detecting low photon flux are the major focus for the generation of mid-wavelength infrared (MWIR) photodetectors

  • MWIR avalanche photodiode (APD) devices are suitable for the detection in passive imaging of attenuated optical signals due to long-range applications benefiting from the superior transmission of MWIR light through common atmospheric issues

  • In this letter we demonstrate a MWIR APD device based on InAs/InSb superlattice

Read more

Summary

Introduction

Detectors with a capability of detecting low photon flux are the major focus for the generation of mid-wavelength infrared (MWIR) photodetectors. MWIR detector material has shown great potential to be utilized for several applications, such as aerial and satellite reconnaissance, target tracking using a heat signal, object identification, vascular and cancer detection, and industrial process monitoring [3,4,5,6,7]. In most of these applications, there is a need to increase the capability of the system to detect light in a low photon flux situation. MWIR APD devices are suitable for the detection in passive imaging of attenuated optical signals due to long-range applications benefiting from the superior transmission of MWIR light through common atmospheric issues

Objectives
Methods
Results
Conclusion
Full Text
Published version (Free)

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