1980
DOI: 10.1109/t-ed.1980.20048
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Emitter effects in shallow bipolar devices: Measurements and consequences

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Cited by 78 publications
(5 citation statements)
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“…We obtained intrinsic radiative lifetimes of the order of 10 –4 s, almost 3 orders of magnitude shorter than those of bulk cubic Si . These relaxation times are shorter than the experimentally measured Auger lifetimes in bulk cubic Si for a majority carrier density of 10 17 cm –3 , thus in the low carrier concentration limit, radiative decay is predicted to be the dominant recombination mechanism. Increasing the Ge concentration should further shorten these values, as the bandgap narrows and the conduction band minimum acquires a stronger Ge character.…”
mentioning
confidence: 65%
“…We obtained intrinsic radiative lifetimes of the order of 10 –4 s, almost 3 orders of magnitude shorter than those of bulk cubic Si . These relaxation times are shorter than the experimentally measured Auger lifetimes in bulk cubic Si for a majority carrier density of 10 17 cm –3 , thus in the low carrier concentration limit, radiative decay is predicted to be the dominant recombination mechanism. Increasing the Ge concentration should further shorten these values, as the bandgap narrows and the conduction band minimum acquires a stronger Ge character.…”
mentioning
confidence: 65%
“…So far, solar cells have been mostly simulated with empirical BGN models that were derived from electronic measurements 25,[32][33][34][35][36][37][38][39][40][41][42][43] of highly doped silicon, as is shown in Fig. 3.…”
Section: B Apparent Versus Theoretically Derived Band-gap Narrowingmentioning
confidence: 99%
“…(4.2) are set as follows. The coefficient a e in n-doped Si at 300 K is measured to be 1.6 × 10 −31 cm 6 s −1 [40]. It is expected to follow a temperature dependence of T 0.72 [35].…”
Section: Auger Recombination Coefficientmentioning
confidence: 93%