首页> 外文期刊>Journal of Applied Physics >Optical constants and band gap of wurtzite Al1-xScxN/Al2O3 prepared by magnetron sputter epitaxy for scandium concentrations up to x=0.41
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Optical constants and band gap of wurtzite Al1-xScxN/Al2O3 prepared by magnetron sputter epitaxy for scandium concentrations up to x=0.41

机译:磁控溅射外延法制备的钪浓度高达x=0.41的纤锌矿Al1-xScxN/Al2O3的光学常数和带隙

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摘要

Wurtzite Al1-xScxN thin films with scandium Sc concentrations up to x=0.41 were prepared by reactive pulsed DC magnetron co-sputtering at heater temperatures between 300 degrees C and 400 degrees C on Al2O3 substrates. Spectroscopic ellipsometry was used to determine the dielectric functions of wurtzite Al1-xScxN by modeling the spectra with a three-layer model involving parametric oscillator functions for the Al1-xScxN layers. By combining ellipsometry with transmission spectroscopy, we determined the composition dependence of the optical band gap E-g. For x<0.25, the experimentally determined band gap follows the theoretical prediction with an offset, which arises from residual sub-band gap absorption. For higher Sc concentrations, for which the band gap is expected to become indirect, the experimental data deviate from the theoretical values for the direct band gap. No absorption that can be attributed to cubic ScN crystallites was observed up to x=0.41, indicating a high phase purity in line with X-ray diffraction data.
机译:在Al2O3衬底上,采用300°C-400°C加热温度下,采用反应脉冲直流磁控共溅射法制备了钪Sc浓度高达x=0.41的纤锌矿Al1-xScxN薄膜.采用椭圆偏振光谱法确定纤锌矿Al1-xScxN的介电函数,通过涉及Al1-xScxN层参数振荡器函数的三层模型对光谱进行建模。通过椭圆偏振法和透射光谱法相结合,我们确定了光学带隙E-g的成分依赖性。对于 x<0.25,实验确定的带隙遵循理论预测,但有一个偏移,该偏移是由残余子带隙吸收引起的。对于较高的Sc浓度,预计带隙会变为间接,实验数据偏离了直接带隙的理论值。在高达 x=0.41 时未观察到可归因于立方 ScN 微晶的吸收,表明相纯度很高,与 X 射线衍射数据一致。

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