We report on Hg1−xCdxTe mid-wavelength infrared (MWIR) detectors grown by molecular-beam epitaxy (MBE) on CdZnTe substrates. Current-voltage (I-V) characteristics of HgCdTe-MWIR devices and temperature dependence of focal-plane array (FPA) dark current have been investigated and compared with the most recent InSb published data. These MWIR p-on-n Hg1−xCdxTe/CdZnTe heterostructure detectors give outstanding performance, and at 68 K, they are limited by diffusion currents. For temperatures lower than 68 K, in the near small-bias region, another current is dominant. This current has lower sensitivity to temperature and most likely is of tunneling origin. High-performance MWIR devices and arrays were fabricated with median RoA values of 3.96 × 1010 Ω-cm2 at 78 K and 1.27 × 1012 Ω-cm2 at 60 K; the quantum efficiency (QE) without an antireflection (AR) coating was 73% for a cutoff wavelength of 5.3 µm at 78 K. The QE measurement was performed with a narrow pass filter centered at 3.5 µm. Many large-format MWIR 1024 × 1024 FPAs were fabricated and tested as a function of temperature to confirm the ultra-low dark currents observed in individual devices. For these MWIR FPAs, dark current as low as 0.01 e−/pixel/sec at 58 K for 18 × 18 µm pixels was measured. The 1024 × 1024 array operability and AR-coated QE at 78 K were 99.48% and 88.3%, respectively. A comparison of these results with the state-of-the-art InSb-detector data suggests MWIR-HgCdTe devices have significantly higher performance in the 30–120 K temperature range. The InSb detectors are dominated by generation-recombination (G-R) currents in the 60–120 K temperature range because of a defect center in the energy gap, whereas MWIR-HgCdTe detectors do not exhibit G-R-type currents in this temperature range and are limited by diffusion currents.
[1]
Marcia J. Rieke,et al.
256 x 256 HgCdTe focal plane array for the Hubble Space Telescope
,
1990,
Other Conferences.
[2]
James D. Garnett,et al.
Infrared detectors for ground-based and space-based astronomy applications
,
2000,
Astronomical Telescopes and Instrumentation.
[3]
Peter Capper,et al.
Properties of Narrow-Gap Cadmium-Based Compounds
,
1995
.
[4]
Donald N. B. Hall,et al.
Characterization of λc=5 μm Hg:Cd:Te arrays for low-background astronomy
,
2000,
Astronomical Telescopes and Instrumentation.
[5]
Gert Finger,et al.
Infrared detector development programs for the VLT instruments at the European Southern Observatory
,
1998,
Astronomical Telescopes and Instrumentation.
[6]
R. Zucca,et al.
HgCdTe double heterostructure injection laser grown by molecular beam epitaxy
,
1991
.