In this work, we investigate the ability of a newly fabricated metal–semiconductor–metal (MSM) solar-blind ultraviolet (UV) photodetector (PD). Three Al <tex-math notation="LaTeX">X</tex-math> Ga <tex-math notation="LaTeX">1-X</tex-math> N films with different Al content were used to form heterostructures, and different metal stacks were deposited on their two sides to achieve asymmetric contact electrodes. The device exhibited a dark current of 2.53 <tex-math notation="LaTeX">×</tex-math> 10 <tex-math notation="LaTeX">⁻⁸</tex-math> A and a peak responsivity of 2.86 at <tex-math notation="LaTeX">$-$</tex-math> 9 V, while corresponding dark current and peak responsivity at 9 V are 4.90 <tex-math notation="LaTeX">×</tex-math> 10 <tex-math notation="LaTeX">⁻⁷</tex-math> A and 20.19 A/W, respectively. Furthermore, its response speed was faster under reverse bias than forward bias. Two-dimensional device simulations were used to obtain the bias-dependent energy bands, electric fields, and carrier concentrations to explain the discrepancy of detection performances between different bias polarities.
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Dai et al. (2024) studied this question.
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