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利用卤化物气相外延反应器中前驱体比例模型在蓝宝石衬底上生长β-GaO层的研究进展。

Development of β-GaO layers growth on sapphire substrates employing modeling of precursors ratio in halide vapor phase epitaxy reactor.

作者信息

Pozina Galia, Hsu Chih-Wei, Abrikossova Natalia, Kaliteevski Mikhail A, Hemmingsson Carl

机构信息

Department of Physics, Chemistry and Biology (IFM), Linköping University, 581 83, Linköping, Sweden.

St-Petersburg Academic University, Khlopina 8/3, St. Petersburg, Russian Federation, 194021.

出版信息

Sci Rep. 2020 Dec 17;10(1):22261. doi: 10.1038/s41598-020-79154-9.

Abstract

Gallium oxide is a promising semiconductor with great potential for efficient power electronics due to its ultra-wide band gap and high breakdown electric field. Optimization of halide vapor phase epitaxy growth of heteroepitaxial [Formula: see text]-GaO layers is demonstrated using a simulation model to predict the distribution of the ratio of gallium to oxygen precursors inside the reactor chamber. The best structural quality is obtained for layers grown at 825-850 °C and with a III/VI precursor ratio of 0.2. Although the structural and optical properties are similar, the surface morphology is more deteriorated for the [Formula: see text]-GaO layers grown on 5 degree off-axis sapphire substrates compared to on-axis samples even for optimized process parameters. Cathodoluminescence with a peak at 3.3 eV is typical for unintentionally doped n-type [Formula: see text]-GaO and shows the appearance of additional emissions in blue and green region at ~ 3.0, ~ 2.8, ~ 2.6 and ~ 2.4 eV, especially when the growth temperatures is lowered to 800-825 °C. Estimation of the band gap energy to ~ 4.65 eV from absorption indicates a high density of vacancy defects.

摘要

氧化镓是一种很有前景的半导体,因其超宽带隙和高击穿电场而在高效电力电子领域具有巨大潜力。利用模拟模型来预测反应室内镓与氧前驱体的比例分布,展示了异质外延[化学式:见原文]-GaO层的卤化物气相外延生长的优化过程。在825 - 850°C生长且III/VI前驱体比例为0.2的层获得了最佳的结构质量。尽管结构和光学性质相似,但即使对于优化的工艺参数,与轴向样品相比,在5度离轴蓝宝石衬底上生长的[化学式:见原文]-GaO层的表面形貌恶化更严重。对于非故意掺杂的n型[化学式:见原文]-GaO,典型的阴极发光峰值在3.3 eV,并且在3.0、2.8、2.6和2.4 eV的蓝色和绿色区域出现额外发射,特别是当生长温度降至800 - 825°C时。从吸收光谱估计带隙能量约为4.65 eV,表明存在高密度的空位缺陷。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/9628/7746736/460ad372e2d1/41598_2020_79154_Fig1_HTML.jpg

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