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Gigahertz cutoff frequency capabilities of CdHgTe photovoltaic detectors at 10.6 µ
45
Citations
4
References
1972
Year
Thz PhotonicsElectrical EngineeringFinal PhotodiodesEngineeringApplied PhysicsTerahertz ScienceTerahertz TechniqueCdhgte Photovoltaic DetectorsP-n JunctionsPhotoelectric MeasurementShunt ResistanceTerahertz PhotonicsOptoelectronicsPhotovoltaicsSolar Cell Materials
Using departure from stoichiometry, p-n junctions were prepared in Cd <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">x</inf> Hg <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">1-x</inf> Te with <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">x \simeq 0.20</tex> for the study of photovoltaic detection at 10.6 μ. In the final photodiodes, with sensitive areas between <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">4 \times 10^{-4}</tex> and 10 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">-3</sup> cm <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sup> , values such as <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">10^{5} \Omega</tex> and 8 pF have been observed at -0.1 V reverse bias for the shunt resistance and capacitance at 77°K. The CO <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</inf> laser detection characteristics were investigated, leading to 10 <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">10</sup> < D <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">*</sup> (10.6 μ, 1800 Hz, 1 Hz) <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">\leq 5 \times 10^{10}</tex> cm W <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">-1</sup> Hz <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">1/2</sup> , a frequency response flat up to 1 GHz, a heterodyne noise equivalent power (NEP) = <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">8 \times 10^{-20}</tex> W/Hz with l-mW local oscillator power. Studies as a function of the temperature indicated that substantial sensitivity can be obtained up to 135°K.
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