宽间隙材料的光致缺陷:氢化非晶硅-碳和硅-氮薄膜

M. Fathallah, M. Mars, C. Pirri, E. Tresso
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引用次数: 4

摘要

采用13.56 MHz等离子体增强化学气相沉积技术,以SiH4 + C2H2 (+H2)、SiH4 + NH3 (+H2)、SiH4 + NH3 (+H2)混合气体为原料,制备了光学间隙在1.9 ~ 4.0 ev范围内的宽禁带氢化非晶硅碳膜和硅氮膜。通过对沉积条件的选择,获得了器件级的薄膜,并已成功地应用于光电技术。这些薄膜在平均天气条件下太阳光谱(空气质量2.0)中浸泡90小时,监测吸收的能量。对每次损伤发生后的光学性质进行了测量,并利用光热偏转光谱法测定了由于光浸泡引起的缺陷密度演变。在所有样品中观察到,在光照射下缺陷密度的增加与碳或氮气体源、等离子体条件和初始性质密切相关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Photoinduced defects in wide-gap materials: Hydrogenated amorphous silicon-carbon and silicon-nitrogen films
Abstract Wide-bandgap hydrogenated amorphous silicon-carbon and silicon-nitrogen films having optical gaps in the range 1.9–4.0eV have been deposited by the 13.56 MHz plasma-enhanced chemical vapour deposition technique from SiH4 + C2H2 (+H2), SiH4 + NH3 (+H2), gas mixtures. The deposition conditions have been chosen so as to obtain device-quality films already successfully applied in optoelectronic technology. The films have been light soaked in the average weather conditions solar spectrum (air mass 2.0) for times up to 90 h, monitoring the absorbed energy. The optical properties have been measured after each occurrence of damage, and the defect density evolution due to light soaking was determined by photothermal deflection spectroscopy. An increase in the density of defects with light exposure was observed in all samples strongly dependent on carbon or nitrogen gas sources, plasma conditions and initial properties.
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