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

机译:AL_XGA_(1-X)N光阴离子的光学元件结构设计

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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和反射率,透射率和吸收性制备AL_XGA_(1-x)N光电阴极进行测试。基于薄膜原理,构建了T模式AL_XGA_(1-X)N光电病的光学模型,然后模拟了光学性质和量子效率。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”性能的探测器的需求。获得最佳厚度的AL_XGA_(1-x)n层,以获得最高量子效率,并且最佳厚度为0.3μm。吸收性和量子效率之间存在密切关系,与“三步”模型很好。这项工作给出了AL_XGA_(1-X)N光电阴极的设计和准备的参考。

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