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Structural and optical properties of CuGaSe_2 layers grown by the hot wall epitaxy method

机译:热壁外延生长CuGaSe_2层的结构和光学性质

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Copper gallium selenide (CuGaSe_2, CGS) layers were grown by the hot wall epitaxy method. The optimum temperatures of the substrate and source for growth turned out to be 450 and 610 ℃, respectively. The CGS layers were epitaxially grown along the < 110 > direction and consisted of Ga-rich components indicating the slight stoichiometric deviations. Based on the absorption measurement, the band-gap variation of CGS was well interpreted by the Varshni's equation. The band-gap energies at low temperatures, however, had a higher value than those of other CGS. It suggests that the band-gap increase is influenced by the slightly Ga-rich composition. From the low-temperature photoluminescence experiment, sharp and intensive free- and bound-exciton peaks were observed. By analyzing these emissions, a band diagram of the observed optical transitions was obtained. From the solar cell measurement, an 11.17% efficiency on the n-CdS/p-CGS junction was achieved.
机译:通过热壁外延法生长硒化铜镓(CuGaSe_2,CGS)层。衬底和生长源的最佳温度分别为450和610℃。 CGS层沿<110>方向外延生长,由富含Ga的成分组成,表明存在轻微的化学计量偏差。基于吸收测量,Carsni方程很好地解释了CGS的带隙变化。但是,低温下的带隙能量比其他CGS具有更高的值。这表明带隙的增加受略微富含Ga的成分的影响。从低温光致发光实验,观察到尖峰和强烈的自由和束缚激子峰。通过分析这些发射,获得了观察到的光学跃迁的能带图。通过太阳能电池测量,n-CdS / p-CGS结的效率达到了11.11%。

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