首页> 外文期刊>Journal of Physics, D. Applied Physics: A Europhysics Journal >Structural and ellipsometric study on tailored optical properties of tantalum oxynitride films deposited by reactive sputtering
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Structural and ellipsometric study on tailored optical properties of tantalum oxynitride films deposited by reactive sputtering

机译:反应溅射沉积氧氮化钽薄膜的光学特性的结构和椭偏研究

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摘要

Oxynitride materials, which offer the possibility of merging oxide and nitride properties, are increasingly studied for this reason. This paper focuses on assessing the optical properties of tantalum oxynitride thin films deposited by pure tantalum target sputtering in an Ar/O-2/N-2 reactive atmosphere. First, by changing the oxygen to reactive gas flow rate ratio, and using thermal post-treatment, we deposited films with elemental compositions studied by Rutherford backscattering spectroscopy, ranging from a nitride (close to Ta3N5) to an oxide (close to Ta2O5) with various structures analyzed by x-ray diffraction. Their optical properties were investigated in depth by spectroscopic ellipsometry and UV-visible spectroscopy. For the ellipsometry investigation, we propose a model combining the Tauc-Lorentz law and additional Lorentz oscillator: the first contribution is linked to a semi-conductor or insulator film matrix, and the second one to the presence of conductive TaN crystals. Ellipsometry thus appears as a powerful tool to investigate complex materials such as tantalum oxynitrides. Moreover, we demonstrated that using this deposition method we were able to finely tune the film refractive index from 3.4 to 2.0 (at 1.96 eV) and the optical band gap, specifically from 1.3 to 2.7 eV.
机译:由于这个原因,人们越来越多地研究提供氧氮化物材料的可能性,这些氧氮化物材料提供了合并氧化物和氮化物性质的可能性。本文着重评估在Ar / O-2 / N-2反应性气氛中通过纯钽靶溅射沉积的氧氮化钽薄膜的光学性能。首先,通过改变氧气与反应气体的流量比,并进行热后处理,我们沉积了具有卢瑟福背散射光谱研究的元素组成的膜,其成分从氮化物(接近Ta3N5)到氧化物(接近Ta2O5)到通过X射线衍射分析各种结构。通过椭圆偏振光谱法和紫外可见光谱对它们的光学性质进行了深入研究。对于椭偏测量,我们提出了一个结合Tauc-Lorentz定律和其他Lorentz振荡器的模型:第一个贡献与半导体或绝缘膜矩阵有关,第二个与导电TaN晶体有关。椭偏法因此成为研究复杂材料(如氧氮化钽)的有力工具。此外,我们证明了使用这种沉积方法,我们能够将膜的折射率从3.4精确地调整到2.0(在1.96 eV时)和光学带隙,特别是从1.3到2.7 eV。

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