中国物理B ›› 2007, Vol. 16 ›› Issue (2): 553-557.doi: 10.1088/1009-1963/16/2/045
侯国付1, 薛俊明1, 郭群超1, 孙建1, 赵颖1, 耿新华1, 李乙钢2
Hou Guo-Fu(侯国付)a)b)c)†, Xue Jun-Ming(薛俊明)a)b)c), Guo Qun-Chao(郭群超)a)b)c), Sun Jian(孙建)a)b)c), Zhao Ying(赵颖)a)b)c), Geng Xin-Hua(耿新华)a)b)c), and Li Yi-Gang(李乙钢)d)
摘要: The incubation layers in microcrystalline silicon films (\muc-Si:H) are studied in detail. The incubation layers in \muc-Si:H films are investigated by bifacial Raman spectra, and the results indicate that either decreasing silane concentration (SC) or increasing plasma power can reduce the thickness of incubation layer. The analysis of the in-situ diagnosis by plasma optical emission spectrum (OES) shows that the emission intensities of the SiH*(412\,nm) and H_\al (656nm) lines are time-dependent, thus SiH*/H_\al ratio is of temporal evolution. The variation of SiH*/H_\al ratio can indicate the variation in relative concentration of precursor and atomic hydrogen in the plasma. And the atomic hydrogen plays a crucial role in the formation of \muc-Si:H; thus, with the plasma excited, the temporal-evolution SiH*/H_\al ratio has a great influence on the formation of an incubation layer in the initial growth stage. The fact that decreasing the SC or increasing the plasma power can decrease the SiH*/H_\al ratio is used to explain why the thickness of incubation layer can reduce with decreasing the SC or increasing the plasma power.
中图分类号: (Chemical vapor deposition (including plasma-enhanced CVD, MOCVD, ALD, etc.))