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基于超宽带隙 Sn 掺杂β-GaO 微片/MnO 量子点的 p-n 结增强型紫外光光电探测器的光响应率。

Enhanced Photoresponsivity UV-C Photodetectors Using a p-n Junction Based on Ultra-Wide-Band Gap Sn-Doped β-GaO Microflake/MnO Quantum Dots.

机构信息

Physical Sciences and Engineering Division, King Abdullah University of Science and Technology (KAUST), Thuwal23955-6900, Saudi Arabia.

Department of Physics, College of Sciences, Princess Nourah Bint Abdulrahman University (PNU), Riyadh11671, Saudi Arabia.

出版信息

ACS Appl Mater Interfaces. 2023 Mar 8;15(9):12127-12136. doi: 10.1021/acsami.2c18900. Epub 2023 Feb 21.

Abstract

Solar-blind self-powered UV-C photodetectors suffer from low performance, while heterostructure-based devices require complex fabrication and lack p-type wide band gap semiconductors (WBGSs) operating in the UV-C region (<290 nm). In this work, we mitigate the aforementioned issues by demonstrating a facile fabrication process for a high-responsivity solar-blind self-powered UV-C photodetector based on a p-n WBGS heterojunction structure, operating under ambient conditions. Here, heterojunction structures based on p-type and n-type ultra-wide band gap WBGSs (i.e. both are characterized by energy gap ≥4.5 eV) are demonstrated for the first time; mainly p-type solution-processed manganese oxide quantum dots (MnO QDs) and n-type Sn-doped β-GaO microflakes. Highly crystalline p-type MnO QDs are synthesized using cost-effective and facile pulsed femtosecond laser ablation in ethanol (FLAL), while the n-type GaO microflakes are prepared by exfoliation. The solution-processed QDs are uniformly dropcasted on the exfoliated Sn-doped β-GaO microflakes to fabricate a p-n heterojunction photodetector, resulting in excellent solar-blind UV-C photoresponse characteristics (with a cutoff at ∼265 nm) being demonstrated. Further analyses using XPS demonstrate the good band alignment between p-type MnO QDs and n-type β-GaO microflakes with a type-II heterojunction. Superior photoresponsivity (922 A/W) is obtained under bias, while the self-powered responsivity is ∼86.9 mA/W. The fabrication strategy adopted in this study will provide a cost-effective means for the development of flexible and highly efficient UV-C devices suitable for energy-saving large-scale fixable applications.

摘要

基于宽禁带半导体(WBGS)的太阳盲自供电紫外-C 光电探测器存在性能不佳的问题,而异质结构基器件则需要复杂的制造工艺,并且缺乏在紫外-C 波段(<290nm)工作的 p 型 WBGS。在这项工作中,我们通过展示一种基于 p-n WBGS 异质结结构的高响应比太阳盲自供电紫外-C 光电探测器的简易制造工艺来解决上述问题,该探测器在环境条件下运行。在这里,我们首次展示了基于 p 型和 n 型超宽带隙 WBGS(即两者的能隙均≥4.5eV)的异质结构;主要是 p 型溶液处理的锰氧化物量子点(MnO QDs)和 n 型掺 Sn 的β-GaO 微片。使用经济高效且简便的飞秒激光脉冲在乙醇(FLAL)中合成了高度结晶的 p 型 MnO QDs,而 n 型 GaO 微片则通过剥离法制备。将溶液处理的 QDs 均匀地滴落在剥离的掺 Sn 的β-GaO 微片上,以制造 p-n 异质结光电探测器,从而展示了出色的太阳盲紫外-C 光响应特性(截止波长约为 265nm)。进一步的 XPS 分析表明,p 型 MnO QDs 和 n 型β-GaO 微片之间具有良好的能带排列,为 II 型异质结。在偏压下获得了优异的光响应率(922A/W),而自供电响应率约为 86.9mA/W。本研究中采用的制造策略将为开发适合节能大规模固定应用的柔性和高效紫外-C 器件提供一种具有成本效益的方法。

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