2 research outputs found
Ultrasensitive, Superhigh Signal-to-Noise Ratio, Self-Powered Solar-Blind Photodetector Based on <i>n</i>‑Ga<sub>2</sub>O<sub>3</sub>/<i>p</i>‑CuSCN Core–Shell Microwire Heterojunction
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 (R254/R365) 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
A Spiro-MeOTAD/Ga<sub>2</sub>O<sub>3</sub>/Si p‑i‑n Junction Featuring Enhanced Self-Powered Solar-Blind Sensing via Balancing Absorption of Photons and Separation of Photogenerated Carriers
Solar
blind ultraviolet (SBUV) self-powered photodetectors (PDs)
have a great number of applications in civil and military exploration.
Ga2O3 is a prospective candidate for SBUV detection
owing to its reasonable bandgap corresponding to the SBUV waveband.
Nevertheless, the previously reported Ga2O3 photovoltaic
devices had low photoresponse performance and were still far from
the demands of practical application. Herein, we propose an idea of
using spiro-MeOTAD (spiro) as the SBUV transparent conductive layer
to construct p-i-n PDs (p-spiro/Ga2O3/n-Si).
With the aid of double built-in electric fields, the designed p-i-n
PDs could operate without any external power source. Furtherly, the
influence of spiro thickness on improving the photoelectric performance
of devices is investigated in detail and the optimum device is achieved,
translating to a peak responsivity of 192 mA/W upon a weak 254 nm
light illumination of 2 μW/cm2 at zero bias. In addition,
the I–t curve of our PD shows
binary response characteristics and a four-stage current response
behavior under a small forward bias, and also, its underlying working
mechanism is analyzed. In sum, this newly developed device presents
great potential for booming the high energy-efficient optoelectronic
devices in the short run
