Is the Cu/Zn Disorder the Main Culprit for the Voltage Deficit in Kesterite Solar Cells?

Is the Cu/Zn Disorder the Main Culprit for the Voltage Deficit in Kesterite Solar Cells?
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DOI:
10.1002/aenm.201502276
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发表时间:
2016-06-22
影响因子:
27.8
通讯作者:
Dennler, Gilles
Dennler, Gilles
中科院分区:
材料科学1区
文献类型:
--
作者:
Bourdais, Stephane;Chone, Christophe;Dennler, Gilles

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基于锌黄锡矿Cu 2 ZnSn(S-x,Se 1-x)(4)化合物(CZTSSe)的光伏薄膜太阳能电池已达到>12%的太阳光-电转换效率。这与Cu(In 1-y,Gay)Se-2和CdTe母体技术中已知的>20%的记录器件仍然相差甚远。选择文献中报道的>9%的CZTSSe器件进行检查,以回顾过去几年取得的进展。这些器件的开路电压(V-oc)很低,从未超过V-oc(max)的60%,这是根据肖克利-奎塞尔辐射极限(S-Q极限)预期的。阴离子(S/Se)的分布和阳离子(Cu/Zn)的障碍上的V-OC赤字和最终的光伏性能的锌黄锡矿设备的可能的作用,在这里澄清。虽然S/Se阴离子分布预期对于任何比率X都是均匀的,但是可以发现在较大面积上的一些颗粒与颗粒和其他不均匀性,如在我们的CZTSSe膜上量化的。然而,这些阴离子分布可被认为对V-oc不足具有可忽略的影响。在Cu/Zn有序侧,尽管可以观察到显著的带隙变化(>10%),但从实验设备和计算中得出类似的结论,仍然在辐射S-Q限制内。的影响和未来的改进方式进行了讨论。
Photovoltaic thin film solar cells based on kesterite Cu2ZnSn(S-x, Se1-x)(4) compounds (CZTSSe) have reached >12% sunlight-to-electricity conversion efficiency. This is still far from the >20% record devices known in Cu(In1-y,Gay)Se-2 and CdTe parent technologies. A selection of >9% CZTSSe devices reported in the literature is examined to review the progress achieved over the past few years. These devices suffer from a low open-circuit voltage (V-oc) never better than 60% of the V-oc (max), which is expected from the Shockley-Queisser radiative limit (S-Q limit). The possible role of anionic (S/Se) distribution and of cationic (Cu/Zn) disorder on the V-oc deficit and on the ultimate photovoltaic performance of kesterite devices, are clarified here. While the S/Se anionic distribution is expected to be homogeneous for any ratio x, some grain-to-grain and other non-uniformity over larger area can be found, as quantified on our CZTSSe films. Nevertheless, these anionic distributions can be considered to have a negligible impact on the V-oc deficit. On the Cu/Zn order side, even though significant bandgap changes (>10%) can be observed, a similar conclusion is brought from experimental devices and from calculations, still within the radiative S-Q limit. The implications and future ways for improvement are discussed.