Solar-blind
photodetectors have captured intense attention due
to their high significance in ultraviolet astronomy and biological
detection. However, most of the solar-blind photodetectors have not
shown extraordinary advantages in weak light signal detection because
the forewarning of low-dose deep-ultraviolet radiation is so important
for the human immune system. In this study, a high-performance solar-blind
photodetector is constructed based on the n-Ga2O3/p-CuSCN core–shell microwire
heterojunction by a simple immersion method. In comparison with the
single device of the Ga2O3 and CuSCN, the heterojunction
photodetector demonstrates an enhanced photoelectric performance with
an ultralow dark current of 1.03 pA, high photo-to-dark current ratio
of 4.14 × 104, and high rejection ratio (R
254/R
365) of 1.15 × 104 under a bias of 5 V. Excitingly, the heterostructure photodetector
shows high sensitivity to the weak signal (1.5 μW/cm2) of deep ultraviolet and high-resolution detection to the subtle
change of signal intensity (1.0 μW/cm2). Under the
illumination with 254 nm light at 5 V, the photodetector shows a large
responsivity of 13.3 mA/W, superb detectivity of 9.43 × 1011 Jones, and fast response speed with a rise time of 62 ms
and decay time of 35 ms. Additionally, the photodetector can work
without an external power supply and has specific solar-blind spectrum
selectivity as well as excellent stability even through 1 month of
storage. Such prominent photodetection, profited by the novel geometric
construction and the built-in electric field originating from the p–n heterojunction, meets greatly
well the “5S” requirements of the photodetector for
practical application.
By acting as the trapping centers during change carrier transfer, the oxygen vacancy (VO) plays a critical role in oxide photoelectric devices. Herein, a post-annealing method was introduced to perfect...
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