1983
DOI: 10.1016/0038-1101(83)90004-7
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Grain boundary barrier height in base and space charge regions

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1986
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Cited by 17 publications
(7 citation statements)
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“…(iii) Grain boundary recombination is negligible in the heavily doped emitter [9] and in the space charge region [10]. This is in agreement with Green [11].…”
Section: Physical Model Of An Elementary Solar Cellsupporting
confidence: 65%
See 1 more Smart Citation
“…(iii) Grain boundary recombination is negligible in the heavily doped emitter [9] and in the space charge region [10]. This is in agreement with Green [11].…”
Section: Physical Model Of An Elementary Solar Cellsupporting
confidence: 65%
“…According to this model, the thickness of these regions is W e , W and W b respectively. The following considerations have been introduced in order to simplify our model: (i) The grains are considered as columnar and perpendicular to the n + -p junction [9], and their electrical properties are homogeneous (doping concentration, minority carrier mobility, lifetime and diffusion length).…”
Section: Physical Model Of An Elementary Solar Cellmentioning
confidence: 99%
“…Dugas et al 8 used the quasiequilibrium assumption to examine the barrier heights of grain boundaries in base and space charge regions. Despite this simplification they conclude that grain boundaries passing through p-n junctions can lead to significant grain boundary recombination of excess minority carriers.…”
Section: Review Of Past Modelsmentioning
confidence: 99%
“…• Grain boundary recombination is negligible in the emitter [8] and in the space charge region [9] due to their small thickness.…”
Section: A Physical Model Of An Elementary Solar Cellmentioning
confidence: 99%