材料科学
非晶硅
硅
无定形固体
图层(电子)
带隙
沉积(地质)
纳米晶硅
硅烷
晶体硅
光电子学
太阳能电池
复合材料
化学
结晶学
古生物学
生物
沉积物
作者
Michael Stückelberger,A. Billet,Yannick Riesen,Mathieu Boccard,Matthieu Despeisse,Jan‐Willem Schüttauf,Franz‐Josef Haug,Christophe Ballif
摘要
Abstract We investigate the influence of the deposition parameters for intrinsic amorphous silicon absorber layers on light‐induced degradation (LID) of thin‐film silicon solar cells. The focus is on absorber layers with different bandgaps: on one side, solar cells with a wide‐bandgap absorber layer that provides open‐circuit voltages up to 1.04V; on the other, cells with short‐circuit current densities of 18.2mA/cm 2 with a 300‐nm‐thick narrow‐bandgap absorber layer, and 20mA/cm 2 at reverse bias for a cell with a 1000‐nm‐thick absorber layer. Between these extremes, we varied the hydrogen‐to‐silane ratio and the deposition pressure during the absorber layer deposition. The light‐induced degradation of these materials—covering the deposition regimes of low‐pressure, protocrystalline, polymorphous, and high‐pressure amorphous silicon—incorporated in single‐junction amorphous silicon solar cells is detailed here. For each pressure, we found an optimum hydrogen dilution with least LID close to the amorphous‐to‐microcrystalline transition. The relative LID is similar for all pressures at optimized hydrogen dilutions. Further, we present the influence of absorber layer thickness, p ‐layer thickness, and deposition rate on the kinetics of light‐induced degradation to facilitate the choice of a material for its application in several types of multi‐junction thin‐film silicon solar cells. We show that the degradation kinetics depends, in semi‐logarithmic scale, only weakly on time but more on deposition conditions. Copyright © 2014 John Wiley & Sons, Ltd.
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