Wan Qiyi, Zhang Anzhen, Cao Weiwei, Bai Yonglin, Wang Bo, Cheng Hang, Wang Gang
Opt Express. 2024 Aug 26;32(18):32322-32335. doi: 10.1364/OE.531784.
In this study, a (400) crystal-oriented β-GaO thin film with a thickness of approximately 400 nm was grown on a c-plane sapphire substrate using atomic layer deposition. Schottky contact-type metal-semiconductor-metal solar-blind ultraviolet detectors with an Au/Ni/GaO/Ni/Au structure were fabricated on the epitaxial thin films. The Schottky barrier height is about 1.1 eV. The device exhibited a high responsivity of up to 800 A/W, and a detectivity of 6 × 10 Jones while maintaining a relatively fast response speed with a rise time of 4 ms and a fall time of 12 ms. The photo-to-dark current ratio was greater than 10, and the external quantum efficiency exceeded 10, indicating a significant gain in the device. Through the analysis of TCAD simulation and experimental results, it is determined that the impact ionization at the edge of the MSM electrode and channel contact is the main source of gain. Barrier tunneling effects and the photoconductive effect due to different carrier mobilities were not the primary reasons for the gain.
在本研究中,使用原子层沉积在c面蓝宝石衬底上生长了厚度约为400nm的(400)晶向β-GaO薄膜。在该外延薄膜上制备了具有Au/Ni/GaO/Ni/Au结构的肖特基接触型金属-半导体-金属日盲紫外探测器。肖特基势垒高度约为1.1eV。该器件表现出高达800A/W的高响应度以及6×10琼斯的探测率,同时保持相对较快的响应速度,上升时间为4ms,下降时间为12ms。光电流与暗电流之比大于10,外部量子效率超过10,表明该器件有显著增益。通过对TCAD模拟和实验结果的分析,确定MSM电极边缘与沟道接触处的碰撞电离是增益的主要来源。势垒隧穿效应以及由于不同载流子迁移率导致的光电导效应并非增益的主要原因。