2018
DOI: 10.1109/jstqe.2017.2737880
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Avalanche Photodiodes Based on the AlInAsSb Materials System

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Cited by 35 publications
(13 citation statements)
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“…While a material such as InAs 11 has a very large α/β ratio, it also has a very narrow band-gap and cannot be grown lattice matched to InP. Recent publications have suggested that the AlInAsSb 12 , 13 alloy also may have a large α/β ratio (~50–100), based on the evidence of very low excess noise measurements in thick avalanching structures. This alloy has a relatively large band-gap (at the higher aluminium mole fractions) with low dark currents at room temperature but it needs to be grown on more expensive GaSb substrates.…”
Section: Introductionmentioning
confidence: 99%
“…While a material such as InAs 11 has a very large α/β ratio, it also has a very narrow band-gap and cannot be grown lattice matched to InP. Recent publications have suggested that the AlInAsSb 12 , 13 alloy also may have a large α/β ratio (~50–100), based on the evidence of very low excess noise measurements in thick avalanching structures. This alloy has a relatively large band-gap (at the higher aluminium mole fractions) with low dark currents at room temperature but it needs to be grown on more expensive GaSb substrates.…”
Section: Introductionmentioning
confidence: 99%
“…Fig. 5c shows that the Fe results at M = 10 in these AlAsSb structures, compared with other materials such as Si [27], AlInAs [28] and AlInAsSb [14]. Only InAs [29] appears capable of giving a significantly lower value of excess noise.…”
Section: Excess Noisementioning
confidence: 86%
“…Unfortunately, this small bandgap means room temperature operation of these devices is not possible and some form of cooling is required to reduce their dark currents. Recently, Campbell et al [14,15] showed that the AlInAsSb alloy had a small β/α ratio and excess noise that was comparable to, or superior to that of silicon. This material has a large bandgap of 1.24 eV and can operate at room temperature, however it has to be grown lattice matched on GaSb substrates.…”
Section: Introductionmentioning
confidence: 99%
“…4(a)). With increased reverse bias, a surge in photocurrent was observed at $À2 V, which plateaued at À3 V. This is a typical signature of punch-through voltage or unity gain point 35 corresponding to the depletion region extending to the absorption region edge. Therefore, À3 V was considered the unity gain (UG) point providing a conservative estimate to avoid overestimating the gain in our NW APDs.…”
Section: Current-voltage (I-v) Measurementsmentioning
confidence: 94%