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New InGaAs/InP avalanche photodiode structure for the 1-1.6 µm wavelength region
93
Citations
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References
1980
Year
PhotonicsElectrical EngineeringShort Wavelength OpticEngineeringPhysicsOptical PropertiesApplied PhysicsNew Lighting TechnologyPhotoelectric MeasurementMultiplication Noise PowerSynchrotron RadiationCurrent Multiplication FactorM Wavelength RegionOptoelectronicsBreakdown Voltage
Low dark current and low multiplication noise properties for an In <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0.53</inf> Ga <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0.47</inf> As/InP avalanche photodiode are described. The diode is prepared with an In <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0.53</inf> Ga <inf xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">0.47</inf> As light absorption layer and an InP avalanche multiplication region. The lowest dark current density of <tex xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">5.2 \times 10^{-4}</tex> A/cm <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sup> is obtained at 90 percent of a breakdown voltage. Multiplication noise power is proportional to the 2.7th power of the current multiplication factor. Impact ionization coefficient by holes is larger by 2-3 times than that by electrons in
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