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超敏感和超快速自动供电的紫外线光探测器阵列用于太阳盲和弱光成像
Weilong Deng1, Xiangyu Fan2, Yuxuan Du2
1National Key Laboratory of Science and Technology on Advanced Composites in Special Environments, Harbin Institute of Technology, Harbin, 150001, China.
Advanced materials (Deerfield Beach, Fla.)
|October 17, 2025
概括
这项研究引入了一种新型的紫外线 (UV) 光探测器阵列,使用CuNiO2/SiC异质连接进行超敏弱光检测. 该设备实现了卓越的性能,在太阳照明下实现实时成像.
科学领域:
- 材料科学 材料科学 材料科学
- 半导体物理 半导体物理
- 光电学是指光电子产品.
背景情况:
- 使用宽带差半导体 (WBGS) 和异构结构的自动供电紫外线 (UV) 光探测器 (PD) 与超敏感和超快弱光检测相扎.
- 现有的基于SiC和Ga2O3的WBGS紫外线PD在灵敏度和响应速度方面存在局限性.
研究的目的:
- 为了展示一个基于CuNiO2/SiC p-n异构连接的8x8紫外线光探测器阵列.
- 为了在太阳盲和弱光检测条件下实现高性能.
- 探索实时成像应用的潜力.
主要方法:
- 使用CuNiO2/SiC p-n异构连接制造一个8x8的紫外线光检测器阵列.
- 设备性能的表征,包括弱光检测极限,响应时间,响应能力和检测能力.
- 分析电荷传输机制,接口质量和光吸收增强.
主要成果:
- 该CuNiO2 / SiC紫外线光检测器阵列实现了4.6nW·mm-2.6的弱光检测极限.
- 演示了45 ns的快速响应时间,104.2 mA·W-1的高响应度,以及3.4 × 1012 斯的检测能力.
- 呈现出低噪声功率密度 (<10-22 A2·Hz-1) 和高切断频率 (5 kHz),性能优于现有的WBGS紫外线PD.
结论:
- 这种CuNiO2/SiC异质连接对于自动供电的紫外线光探测器是非常有效的.
- 该设备的性能归因于高质量的接口,大型内置电场,福勒-诺德海姆道运输和增强的光吸收.
- 开发的紫外线PD阵列可以在太阳照明下实现高对比度实时反射成像.
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