1992
DOI: 10.1109/3.135278
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Effect of dead space on gain and noise in Si and GaAs avalanche photodiodes

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Cited by 117 publications
(92 citation statements)
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“…One of the reasons is that the ionization coefficient ratio k is closer to unity, so the noise due to hole initiated avalanche is lower, as can be observed comparing the p+/n structures in (Biber et al, 2001) and (Stapels et al, 2007). When the doping levels are even higher, the width of the multiplication region is reduced and standard McIntyre theory is no longer adequate to describe the avalanche process because of the dead space effect (Hayat et al, 1992). In this case, the noise factor becomes lower than the one predicted by standard model both for electron-and hole-initiated avalanche, as observed in (Pancheri et al, 2008).…”
Section: P-substratementioning
confidence: 96%
“…One of the reasons is that the ionization coefficient ratio k is closer to unity, so the noise due to hole initiated avalanche is lower, as can be observed comparing the p+/n structures in (Biber et al, 2001) and (Stapels et al, 2007). When the doping levels are even higher, the width of the multiplication region is reduced and standard McIntyre theory is no longer adequate to describe the avalanche process because of the dead space effect (Hayat et al, 1992). In this case, the noise factor becomes lower than the one predicted by standard model both for electron-and hole-initiated avalanche, as observed in (Pancheri et al, 2008).…”
Section: P-substratementioning
confidence: 96%
“…This model has been shown to correctly predict the excess noise factors independently of the width of the multiplication layer. The gain statistics for double-carrier multiplication APDs, in the presence of dead space and a uniform or a nonuniform electric field, have been developed and reported in [2,[10][11][12]. The theory involves recurrence equations of certain intermediate random variables.…”
Section: Theoretical Backgroundmentioning
confidence: 99%
“…With this assumption, Hayat et al [2,[10][11][12] formulated a dead-spacemultiplication theory (DSMT) that permitted the gain, excess noise factor, breakdown probability, breakdown voltage, and gain probability distribution to be determined in the presence of dead space. Because the DSMT developed in [11] incorporates a nonuniform electric field, it can accommodate arbitrary history-dependent ionization coefficients.…”
Section: Introductionmentioning
confidence: 99%
“…Assuming Poisson photon statistics, the signal-to-noise ratio (SNR) of the total charge accumulation in the detection circuit in a time interval T is given by [17] …”
Section: Performance Factormentioning
confidence: 99%