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首页> 外文期刊>International Journal of Photoenergy >In SituandEx SituStudies of Molybdenum Thin Films Deposited by rf and dc Magnetron Sputtering as a Back Contact for CIGS Solar Cells
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In SituandEx SituStudies of Molybdenum Thin Films Deposited by rf and dc Magnetron Sputtering as a Back Contact for CIGS Solar Cells

机译:射频和直流磁控溅射作为CIGS太阳能电池的背触点沉积的钼薄膜的In Situ和Ex Situ研究

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Molybdenum thin films were deposited by rf and dc magnetron sputtering and their properties analyzed with regards to their potential application as a back contact for CIGS solar cells. It is shown that both types of films tend to transition from tensile to compressive strain when the deposition pressure increases, while the conductivity and the grain size decreas. The nucleation of the films characterized byin situand real time spectroscopic ellipsometry shows that both films follow a Volmer-Weber growth, with a higher surface roughness and lower deposition rate for the rf deposited films. The electronic relaxation time was then extracted as a function of bulk layer thickness for rf and dc films by fitting each dielectric function to a Drude free-electron model combined with a broad Lorentz oscillator. The values were fitted to a conical growth mode and demonstrated that the rf-deposited films have already smaller grains than the dc films when the bulk layer thickness is 30 nm.
机译:通过射频和直流磁控溅射沉积钼薄膜,并就其潜在用途作为CIGS太阳能电池的背接触件进行了性能分析。结果表明,当沉积压力增加时,两种类型的膜都趋于从拉伸应变转变为压缩应变,而电导率和晶粒尺寸则下降。用原位和实时光谱椭圆偏振法表征的膜的成核表明,两个膜都遵循Volmer-Weber生长,对于rf沉积的膜具有较高的表面粗糙度和较低的沉积速率。然后,通过将每个介电函数拟合为与宽Lorentz振荡器结合的Drude自由电子模型,来提取电子弛豫时间与RF和DC膜的体层厚度的关系。将该值拟合为锥形生长模式,并证明当体层厚度为30μnm时,rf沉积膜的晶粒已经比dc膜小。

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