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中国物理学会期刊

具有高光响应度与外量子效率的CsPbIBr2/Ga2O3范德瓦耳斯异质结自供电探测器

Self-powered CsPbIBr2/Ga2O3 van der Waals heterojunction with high responsivity and large external quantum efficiency

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  • 本文报道了一种基于CsPbIBr2/Ga2O3范德瓦耳斯异质结的自供电深紫外光电探测器,该器件通过等离子体增强化学气相沉积(PECVD)和热滴注法(hot-casting)结合制备. X射线衍射和扫描电子显微镜表征证实了β-Ga2O3与CsPbIBr2的薄膜质量. 并通过Tauc曲线得出Ga2O3和CsPbIBr2的光学带隙分别为4.75 eV和2.03 eV. 根据安德森法则(Anderson's rule)证实了该范德瓦耳斯异质结为具有稳定界面内建电场的II型能带排列. 该器件在 10 V偏压下具有极低的暗电流密度(2.09×10-10 A/cm2)以及高达4.01×103的光暗电流比. 得益于界面处的内建电场,该探测器在零偏压下实现了稳定且可重复的光响应,展现出优异的自供电能力. 在 254 nm深紫外光照射及10 V偏压下,该探测器获得了0.17 A/W的光响应度、85%的外量子效率,以及高达2.98×1012 Jones的比探测率. 综上,本研究为高性能自供电日盲紫外光电探测提供了一种可借鉴的路径.

     

    In this work, a self-powered deep ultraviolet photodetector is introduced based on a CsPbIBr2/Ga2O3 van der Waals heterojunction, fabricated via PECVD and hot-casting methods. The crystalline structure and sharp interface were comprehensively verified using X-ray diffraction (XRD) and scanning electron microscopy (SEM), showing a smooth, defect-reduced heterojunction profile with film thicknesses of ~22.52 μm for CsPbIBr2 and ~163.88 μm for Ga2O3. Tauc plots verify bandgaps of 4.75 eV for Ga2O3 and 2.03 eV for CsPbIBr2. According to Anderson’s rule, the CsPbIBr2/Ga2O3 heterojunction forms a typical Type-II band alignment with conduction and valence band offsets of 0.68 eV (ΔEc) and 2.90 eV (ΔEv), which creates a robust built-in electric field across the space charge region to drive efficient photogenerated charge separation. The device delivers ultralow dark current of 1.045×10-11 A at 10 V and a high photo-to-dark current ratio of 4.01×103. Benefiting from the intrinsic built-in potential, stable repeatable photoresponse is realized at zero bias, demonstrating self-powered detection capability. At 10 V bias, the detector achieves a high responsivity of 0.17 A/W, an external quantum efficiency of 85% and an ultrahigh specific detectivity of 2.98×1012 Jones under 254 nm illumination. Furthermore, transient photoresponse measurements demonstrate rapid response performance at zero bias, characterized by rising and decaying processes of 0.53 s and 0.33 s, respectively. In all, this work offers a facile strategy for high-performance self-powered solar-blind UV photodetection.

     

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