晶界不是铜(In,Ga)Se2 吸收体中乌尔巴赫尾迹的来源

S. Gharabeiki, Muhammad Uzair Farooq, Taowen Wang, Mohit Sood, M. Melchiorre, Christian Kaufmann, A. Redinger, S. Siebentritt
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摘要

Cu(In,Ga)Se2(CIGSe)吸收体中乌尔巴赫尾态的存在已被确定为 CIGSe 太阳能电池性能的限制因素。尾态有助于辐射和非辐射重组过程,最终导致开路电压(VOC)降低,进而降低 CIGSe 器件的整体效率。乌巴赫尾迹是由结构和热失调引起的。乌巴赫尾迹可以用乌巴赫能量来表征,乌巴赫能量与尾态的大小有关。在多晶 CIGSe 吸收体中,晶界可被视为结构紊乱,因此有可能导致乌巴赫尾迹。事实上,有人认为晶界处的带弯曲对尾态有很大的影响。本研究重点考察了乌巴赫尾态与晶界带弯曲之间的相关性。从光致发光(PL)测量中提取了 CIGSe 样品的 Urbach 能量,结果表明,在材料中引入钠(Na)可以降低 Urbach 能量,而通过 RbF 沉积后处理(PDT)可以进一步降低 Urbach 能量。开尔文探针力显微镜 (KPFM) 测量对晶界处的带弯曲进行了研究。对 340 多个晶界进行的全面统计分析显示,乌巴赫尾与晶界之间没有任何相关性。我们在热能(室温下为 26meV)范围内测量到了晶界处较小的带弯曲值。此外,我们与强度相关的 PL 测量结果表明,乌巴赫尾至少部分是静电位波动的结果。这支持了这样一个模型,即碱元素的引入主要降低了静电位波动的幅度,从而导致乌巴赫能随之降低。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Grain boundaries are not the source of Urbach tails in Cu(In,Ga)Se2 absorbers
The presence of Urbach tails in Cu(In,Ga)Se2 (CIGSe) absorbers has been identified as a limiting factor for the performance of the CIGSe solar cells. The tail states contribute to both radiative and non-radiative recombination processes, ultimately leading to a reduction in the open-circuit voltage (VOC) and, consequently, decreasing the overall efficiency of CIGSe devices. Urbach tails result from structural and thermal disorders. The Urbach tails can be characterized by the Urbach energy, which is associated with the magnitude of the tail states. Within polycrystalline CIGSe absorbers, grain boundaries can be considered as structural disorder and, therefore, can potentially contribute to the Urbach tails. In fact, it has been proposed that the band bending at grain boundaries contribute significantly to the tail states. This study focuses on examining the correlation between Urbach tails and the band bending at the grain boundaries. The Urbach energies of the CIGSe samples are extracted from photoluminescence (PL) measurements, which reveal that the introduction of Sodium (Na) into the material can lead to a reduction in the Urbach energy, and an even further decrease can be achieved through the RbF post-deposition treatment (PDT). The band bending at the grain boundaries is investigated by Kelvin probe force microscopy (KPFM) measurements. A thorough statistical analysis of more than 340 grain boundaries does not show any correlation between Urbach tails and grain boundaries. We measure small band bending values at the grain boundaries, in the range of the thermal energy (26meV at room temperature). Furthermore, our intensity dependent PL measurements indicate that Urbach tails are, at least in part, a result of electrostatic potential fluctuations. This supports the model that the introduction of alkali elements mainly decreases the magnitude of electrostatic potential fluctuations, resulting in a subsequent reduction in the Urbach energy.
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