Observation of photoelectric-induced microplasma avalanche breakdown in AlGaN ultraviolet photodiode with separate absorption and multiplication structure

Author:

Cao Jiying1ORCID,Cai Qing1ORCID,You Haifan1ORCID,Shao Pengfei1ORCID,Wang Jin2,Guo Hui1,Xue Junjun2,Liu Bin1ORCID,Xie Zili1,Cao Xun1ORCID,Lu Hai1ORCID,Zheng Youdou1,Zhang Rong134ORCID,Chen Dunjun1ORCID

Affiliation:

1. Key Laboratory of Advanced Photonic and Electronic Materials, School of Electronic Science and Engineering, Nanjing University 1 , Nanjing 210093, China

2. School of Electronic Science and Engineering, Nanjing University of Posts and Telecommunications 2 , Nanjing 210023, China

3. Collaborative Innovation Center for Optoelectronic Semiconductors and Efficient Devices, Department of Physics, Xiamen University 3 , Xiamen 361005, China

4. Institute of future display technology, Tan Kah Kee Innovation Laboratory 4 , Xiamen 361102, China

Abstract

Amplification of weak ultraviolet signals has always been a challenging issue to design and fabricate high-performance ultraviolet photodetectors. Here, we observe a distinctive microplasma breakdown behavior in AlGaN-based ultraviolet avalanche photodiodes with artificial mesa architecture. At 107 V breakdown voltage, the photocurrent increases sharply whereas dark current intriguingly remains at the extremely low level of 0.1 nA as the applied voltage increases. Simultaneously, a significant blue luminescence phenomenon is observed at the mesa edge of photodiode at breakdown voltage, indicating the occurrence of microplasma breakdown. Ultimately, the microplasma avalanche photodiode achieves a record-high avalanche gain of 3 × 106 with light–dark current ratio readily exceeding 107. Kelvin probe force microscopy was employed to reveal the physical mechanism of localized avalanche breakdown induced by photoelectric effects and elaborate the microplasma discharge process, which is related to surface states. The unprecedented detection mode of photocurrent triggering avalanche events while remaining low dark current is anticipated to effectively shield the background noise and amplify ultraviolet signals. It is worth further research to explore its possibility on high-sensitivity ultraviolet photodetection.

Funder

National Key Research and Development Program of China

National Natural Science Associate Foundation

Key Project of Jiangsu Province, China

National Natural Science Foundation of China

China Postdoctoral Science Foundation

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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