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通过在平面蓝宝石衬底上插入种子层的射频磁控溅射增强型氧化镓薄膜紫外探测器。

Enhancing-GaO-film ultraviolet detectors via RF magnetron sputtering with seed layer insertion on-plane sapphire substrate.

作者信息

Wang Guodong, Wang Haohan, Chen Tingyu, Feng Yanji, Zeng Hua, Guo Lanlan, Liu Xiaolian, Yang Yingli

机构信息

School of Physics and Electronic Information Engineering, Henan Polytechnic University, Jiaozuo, 454003, People's Republic of China.

Instrumental Analysis Center, Henan Polytechnic University, Jiaozuo, 454003, People's Republic of China.

出版信息

Nanotechnology. 2023 Dec 12;35(9). doi: 10.1088/1361-6528/ad0f57.

Abstract

Gallium oxide (GaO) possesses a band gap of approximately 4.9 eV, aligning its detection wavelength within the solar-blind region, making it an ideal semiconductor material for solar-blind photodetectors. This study aims to enhance the performance of GaOultraviolet (UV) detectors by pre-depositing a GaOseed layer on a-plane sapphire substrate. The x-ray diffraction and x-ray photoelectron spectroscopy analyses validated that the deposited films, following high-temperature annealing, comprised-GaO. Comparing samples with and without a 20 nm seed layer, it was found that the former exhibited fewer oxygen defects and substantially improved crystal quality. The incorporation of the seed layer led to the realization of detectors with remarkably low dark current (≤15.3 fA). Moreover, the photo-to-dark current ratio was enhanced by 30% (surpassing 1.3 × 10) and the response/recovery time reduced to 0.9 s/0.01 s, indicating faster performance. Furthermore, these detectors demonstrated higher responsivity (4.8 mA W), improved detectivity (2.49 × 10Jones), and excellent solar-blind characteristics. This study serves as a foundational stepping toward achieving high-quality-GaOthin film and UV detector arrays.

摘要

氧化镓(GaO)的带隙约为4.9电子伏特,其探测波长处于日盲区域内,这使其成为日盲光电探测器的理想半导体材料。本研究旨在通过在a面蓝宝石衬底上预沉积GaO籽晶层来提高GaO紫外(UV)探测器的性能。X射线衍射和X射线光电子能谱分析证实,高温退火后的沉积薄膜由β-GaO组成。对比有无20纳米籽晶层的样品发现,前者的氧缺陷更少,晶体质量显著提高。籽晶层的引入使得探测器实现了极低的暗电流(≤15.3飞安)。此外,光电流与暗电流之比提高了30%(超过1.3×10),响应/恢复时间缩短至0.9秒/0.01秒,表明性能更快。此外,这些探测器表现出更高的响应度(4.8毫安/瓦)、更高的探测率(2.49×10琼斯)以及优异的日盲特性。本研究为实现高质量β-GaO薄膜和紫外探测器阵列奠定了基础。

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