2010
DOI: 10.1016/j.egypro.2010.07.033
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Comparison of a-SiC:H and a-SiN:H as candidate materials for a p-i interface layer in a-Si:H p-i-n solar cells

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Cited by 9 publications
(4 citation statements)
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“…The absorption coefficient of nc-Si:H is about one order of magnitude higher than that of a-SiC:H in the visible part of the sun spectrum. This is in conjunction with the poor absorption property of a-SiC:H due to carbon-induced defects, as reported in the experimental work [33]. However, the absorption coefficient is less for nc-Si:H when compared with a-Si:H, and this translates into the reduced parasitic absorption in nc-Si:H window layer.…”
Section: Resultssupporting
confidence: 61%
See 1 more Smart Citation
“…The absorption coefficient of nc-Si:H is about one order of magnitude higher than that of a-SiC:H in the visible part of the sun spectrum. This is in conjunction with the poor absorption property of a-SiC:H due to carbon-induced defects, as reported in the experimental work [33]. However, the absorption coefficient is less for nc-Si:H when compared with a-Si:H, and this translates into the reduced parasitic absorption in nc-Si:H window layer.…”
Section: Resultssupporting
confidence: 61%
“…The band gap of 2.0 eV for nc‐Si:H layer presents significant energy barrier for electrons, thus reducing recombination at an anode. The absorption coefficient profiles of three different materials have been extracted from different experimental work reported in the literature [21, 27, 33]. The absorption coefficient of nc‐Si:H is about one order of magnitude higher than that of a‐SiC:H in the visible part of the sun spectrum.…”
Section: Resultsmentioning
confidence: 99%
“…These parameters were obtained by the lower (5 sccm) silane gas flow and with 25% ammonia gas fraction. A similar trend was found by Vet et al [ 44 ] who deposited SiNx:H layers by the same method, varying the gas ratio of silane while the amount of ammonia gas was fixed. In accordance with the results of Jasruddin et al, they have found that while the silane gas flow was decreased, the optical band gap was increased.…”
Section: Chemical Vapor Depositionsupporting
confidence: 83%
“…This material has a wide optical band gap (1.7 eV to 2 eV), low growth temperature (~ 200 o C) and can be grown on glass substrates that are cheap and abundant [1]. In addition, a-Si:H also has a high absorption capability in the visible light spectrum [2]. However, the efficiency of a-Si:H-based solar cells is still smaller than the efficiency of crystalline silicon and some other solar cells [3].…”
Section: Introductionmentioning
confidence: 99%