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Design of Optical Component Structure for Al_xGa_(1-x)N photocathodes

机译:Al_xGa_(1-x)N光电阴极的光学组件结构设计

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Al_xGa_(1-x)N photocathode was prepared by MOCVD and the reflectivity, transmittance, and absorptivity were test. Based on thin film principle, optical model of t-mode Al_xGa_(1-x)N photocathodes was built, and then optical properties and quantum efficiencies were simulated. Results show that Al_xGa_(1-x)N photocathodes satisfy the need of detectors with "solar blind" property when the Al component is larger than 0.250. There is an optimal thickness of Al_xGa_(1-x)N layer to obtain highest quantum efficiency, and the optimal thickness is 0.3μm. There is close relation between absorptivity and quantum efficiency, which is in good agreement with the "three-step" model. This work gives a reference for the design and preparation of Al_xGa_(1-x)N photocathodes.
机译:通过MOCVD制备Al_xGa_(1-x)N光电阴极,并测试其反射率,透射率和吸收率。基于薄膜原理,建立了t型Al_xGa_(1-x)N光阴极的光学模型,并对其光学性质和量子效率进行了模拟。结果表明,当Al组分大于0.250时,Al_xGa_(1-x)N光电阴极满足具有“太阳盲”特性的探测器的需求。为了获得最高的量子效率,存在最佳的Al_xGa_(1-x)N层厚度,并且最佳厚度为0.3μm。吸收率与量子效率之间有着密切的关系,这与“三步法”模型非常吻合。这项工作为Al_xGa_(1-x)N光电阴极的设计和制备提供了参考。

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