Enhanced Performance of Self-Powered Solar-Blind Deep UV Photodetectors Based on ZnGa2O4/Ga2O3 Heterojunctions
Self-powered ultraviolet (UV) photodetectors (PDs) attract much research attention because of their promising application in solar-blind region detection. Here, a high-performance self-powered PD is constructed using the heterojunction of gallium oxide (Ga2O3) and ZnGa2O4. Taking advantage of the lo...
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Published in | IEEE sensors journal Vol. 24; no. 11; pp. 17661 - 17668 |
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Main Authors | , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
New York
IEEE
01.06.2024
The Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Subjects | |
Online Access | Get full text |
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Summary: | Self-powered ultraviolet (UV) photodetectors (PDs) attract much research attention because of their promising application in solar-blind region detection. Here, a high-performance self-powered PD is constructed using the heterojunction of gallium oxide (Ga2O3) and ZnGa2O4. Taking advantage of the low concentration of oxygen vacancies (Vo) in ZnGa2O4 and the photovoltaic effect at the interface, the PD demonstrates inspiring solar-blind UV photodetection capabilities. Under external bias (5 V), the ZnGa2O4/Ga2O3 heterojunction PD exhibits an ultralow dark current of 0.06 pA, a high photo-dark current ratio (PDCR) of <inline-formula> <tex-math notation="LaTeX">9.39\times 10^{{5}} </tex-math></inline-formula>, and a rapid response speed. In the self-powered mode (0 V), the PD demonstrates a significant photovoltaic effect, which is characterized to have an open-circuit voltage of 0.14 V. Additionally, it exhibits enhanced photoresponse with PDCR of approximately <inline-formula> <tex-math notation="LaTeX">10^{{4}} </tex-math></inline-formula> (<inline-formula> <tex-math notation="LaTeX">500~\mu </tex-math></inline-formula>W/cm<inline-formula> <tex-math notation="LaTeX">^{{2}}\text {)} </tex-math></inline-formula>. Our findings suggest that ZnGa2O4/Ga2O3 heterojunction PDs can potentially become a highly efficient and energy-saving option for solar-blind detection in the future. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
ISSN: | 1530-437X 1558-1748 |
DOI: | 10.1109/JSEN.2024.3388471 |