• Chinese Optics Letters
  • Vol. 21, Issue 5, 051604 (2023)
Ning Li1, Qingyi Zhang1, Yongtao Yang1, Yuanjun Tang1, Tao Zhang1, Jiaying Shen1, Yuehui Wang1, Fan Zhang1, Yang Zhang2、3、*, and Zhenping Wu1、**
Author Affiliations
  • 1State Key Laboratory of Information Photonics and Optical Communications & School of Science, Beijing University of Posts and Telecommunications, Beijing 100876, China
  • 2Institute of Modern Optics, Nankai University, Tianjin 300071, China
  • 3Tianjin Key Laboratory of Micro-Scale Optical Information Science and Technology, Tianjin 300071, China
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    DOI: 10.3788/COL202321.051604 Cite this Article Set citation alerts
    Ning Li, Qingyi Zhang, Yongtao Yang, Yuanjun Tang, Tao Zhang, Jiaying Shen, Yuehui Wang, Fan Zhang, Yang Zhang, Zhenping Wu. Solar-blind avalanche photodetector based on epitaxial Ga2O3/La0.8Ca0.2MnO3 pn heterojunction with ultrahigh gain[J]. Chinese Optics Letters, 2023, 21(5): 051604 Copy Citation Text show less
    Schematic structure of the β-Ga2O3/LCMO pn junction APD.
    Fig. 1. Schematic structure of the β-Ga2O3/LCMO pn junction APD.
    (a) XRD patterns of β-Ga2O3/LCMO/STO (red line) and LCMO/STO (black line); (b) atomic diagram of cross section in the (100) direction of pn junction.
    Fig. 2. (a) XRD patterns of β-Ga2O3/LCMO/STO (red line) and LCMO/STO (black line); (b) atomic diagram of cross section in the (100) direction of pn junction.
    Solar-blind photoresponse characteristics of Ga2O3/LCMO APD. (a) I-V curves (log scale) in dark and under different light illumination (1–100 µW/cm2). The inset shows the I-V curves enlarged near −37 V. (b) Reverse I-V curves in dark and under 1 µW/cm2 254 nm light intensity; the right axis shows the multiplication gain values. (c) The light intensity-dependent photocurrent and responsivity at a reverse bias of 20 V. (d) Photoresponse spectrum at a reverse bias of 30 V.
    Fig. 3. Solar-blind photoresponse characteristics of Ga2O3/LCMO APD. (a) I-V curves (log scale) in dark and under different light illumination (1–100 µW/cm2). The inset shows the I-V curves enlarged near −37 V. (b) Reverse I-V curves in dark and under 1 µW/cm2 254 nm light intensity; the right axis shows the multiplication gain values. (c) The light intensity-dependent photocurrent and responsivity at a reverse bias of 20 V. (d) Photoresponse spectrum at a reverse bias of 30 V.
    (a) Responsivity; (b) EQE; and (c) LDR of Ga2O3/LCMO pn junction APD under 1 µW/cm2 254 nm UV light intensity as a function of reverse bias.
    Fig. 4. (a) Responsivity; (b) EQE; and (c) LDR of Ga2O3/LCMO pn junction APD under 1 µW/cm2 254 nm UV light intensity as a function of reverse bias.
    CL and valence band XPS energy spectrum of (a) LCMO (∼100 nm)/STO and (b) Ga2O3 (∼300 nm)/LCMO (∼100 nm)/STO; (c) CL XPS energy spectrum of Ga2O3 (∼3 nm)/LCMO (∼100 nm)/STO sample; (d) bandgap of Ga2O3 film; and (e) LCMO film determined by Tauc plots method; (f) band alignment at the Ga2O3/LCMO pn junction.
    Fig. 5. CL and valence band XPS energy spectrum of (a) LCMO (∼100 nm)/STO and (b) Ga2O3 (∼300 nm)/LCMO (∼100 nm)/STO; (c) CL XPS energy spectrum of Ga2O3 (∼3 nm)/LCMO (∼100 nm)/STO sample; (d) bandgap of Ga2O3 film; and (e) LCMO film determined by Tauc plots method; (f) band alignment at the Ga2O3/LCMO pn junction.
    Avalanche multiplication process of Ga2O3/LCMO APD.
    Fig. 6. Avalanche multiplication process of Ga2O3/LCMO APD.
    Ning Li, Qingyi Zhang, Yongtao Yang, Yuanjun Tang, Tao Zhang, Jiaying Shen, Yuehui Wang, Fan Zhang, Yang Zhang, Zhenping Wu. Solar-blind avalanche photodetector based on epitaxial Ga2O3/La0.8Ca0.2MnO3 pn heterojunction with ultrahigh gain[J]. Chinese Optics Letters, 2023, 21(5): 051604
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