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Epitaxial growth of 3C-SiC film by microwave plasma chemical vapor deposition in H2-CH4-SiH4mixtures: Optical emission spectroscopy study
Journal of Vacuum Science & Technology A ( IF 2.9 ) Pub Date : 2021-02-17 , DOI: 10.1116/6.0000745
V. Yu. Yurov 1, 2 , V. G. Ralchenko 1, 2, 3 , A. K. Martyanov 1 , I. A. Antonova 1, 2 , V. S. Sedov 1 , A. A. Khomich 1, 4 , V. V. Voronov 1 , S. S. Savin 5 , M. Y. Shevchenko 1 , A. P. Bolshakov 1
Affiliation  

Microwave (MW) plasma in silane-hydrogen and silane-hydrogen-methane mixtures is used effectively for chemical vapor deposition of Si, SiC, diamond, and SiC-diamond composite films; however, the properties of such plasma at pressures of the order of 100 Torr remain largely unexplored. Here we characterize the MW plasma (2.45 GHz) in SiH4 + H2 and SiH4 + СH4 + H2 mixtures (72 Torr) with silane content ranging from 0% to 5% in the process gas using high-resolution optical emission (OE) spectroscopy. Besides the OE lines of C2 dimer, Balmer series of excited atomic hydrogen (Hα, Hβ, Hγ, Hδ, and Hε), and CH radical, we observed atomic Si lines at 263, 288, and 391 nm and a relatively weak SiH emission. Gas temperature Tg of ≈3160 K is assessed from the rotational structure of the C2 dimer (Δν = 0, λ = 516.5 nm) emission band, and the absorbed microwave power density (MWPD) in the plasma fluctuates in the narrow range between 36 and 43 W/cm3 with a slight tendency to decrease with silane addition. The MWPD, intensity ratio Hα/Hβ of hydrogen Balmer series lines (related to excitation temperature Texc), and Si lines’ intensities in OE spectra as functions of SiH4 concentration in H2 and H2 + CH4 mixtures all show an extremum or a kink in slope near a special point at ≈0.5% SiH4. Finally, we produced a silicon carbide film of cubic polytype 3C-SiC on a (111) oriented Si substrate, which was characterized with Raman spectroscopy and x-ray diffraction, and its monocrystalline structure was confirmed.

中文翻译:

在H2-CH4-SiH4混合物中通过微波等离子体化学气相沉积外延生长3C-SiC膜:发射光谱研究

硅烷-氢和硅烷-氢-甲烷混合物中的微波(MW)等离子可有效地用于化学气相沉积Si,SiC,金刚石和SiC-金刚石复合膜。然而,这种等离子体在100Torr量级的压力下的性质仍未得到充分探索。在这里,我们在的SiH表征MW等离子体(2.45千兆赫)4  + H 2和SiH 4  +СH 4  + H 2分的混合物(72托)与硅烷含量使用高分辨率光学发射范围从0%到工艺气体中的5% (OE)光谱学。除了C的OE线2二聚体,巴尔末串激原子氢(H α,H β,H γ,H δ)和CH自由基,我们观察到263、288和391 nm处的原子Si线以及相对较弱的SiH发射。根据C 2二聚体(Δν= 0,λ= 516.5 nm)发射带的旋转结构估算出大约3160 K的气体温度T g,等离子中吸收的微波功率密度(MWPD)在以下范围之间的狭窄范围内波动: 36 W / cm 3和43 W / cm 3,随硅烷的添加略有降低的趋势。的MWPD,强度比ħ α / H β的氢巴尔末一系列的线(与激励温度Ť EXC),和Si线在OE光谱强度作为SiH与功能4在H +浓度2和H 2  + CH 4的混合物均在≈0.5%SiH 4处的特殊点附近出现极值或扭结。最后,我们在(111)取向的Si衬底上制备了立方多型3C-SiC碳化硅膜,通过拉曼光谱和X射线衍射对其进行了表征,并证实了其单晶结构。
更新日期:2021-03-05
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