Light Harvesting and Charge Recombination in CH3NH3PbI3 Perovskite Solar Cells Studied by Hole Transport Layer Thickness Variation

被引:202
作者
Marinova, Nevena [1 ,2 ]
Tress, Wolfgang [1 ]
Humphry-Baker, Robin [1 ]
Dar, M. Ibrahim [1 ]
Bojinov, Vladimir [2 ,3 ]
Zakeeruddin, Shaik Mohammed [1 ]
Nazeeruddin, Mohammad Khaja [1 ,4 ]
Graetzel, Michael [1 ]
机构
[1] Swiss Fed Inst Technol EPFL, Lab Photon & Interfaces, CH-1015 Lausanne, Switzerland
[2] Univ Chem Technol & Met, Dept Organ Synth, BU-1756 Sofia, Bulgaria
[3] King Abdulaziz Univ, Fac Sci, Dept Chem, Jeddah 21589, Saudi Arabia
[4] King Abdulaziz Univ, CEAMR, Jeddah 21589, Saudi Arabia
关键词
mesoscopic solar cell; spiro-MeOTAD; light-harvesting; electroluminescence; charge recombination; ideality factor; DEPOSITION;
D O I
10.1021/acsnano.5b00447
中图分类号
O6 [化学];
学科分类号
0703 ;
摘要
A tailored optimization of perovskite solar cells requires a detailed understanding of the processes limiting the device efficiency. Here, we study the role of the hole transport layer (HTL) spiro-MeOTAD and its thickness in a mesoscopic TiO2-based solar cell architecture. We find that a sufficiently thick (200 nm) HTL not only increases the charge carrier collection efficiency but also the light harvesting efficiency. This is due to an enhanced reflection of a smooth HTL/Au electrode interface. The rough CH3NH3PbI3 perovskite surface requires an HTL thickness of >400 nm to avoid surface recombination and guarantee a high-Open-circuit voltage. Analyses of the electroluminescence efficiency and the diode ideality factor show that the open-circuit voltage becomes completely limited by trap-assisted recombination in the perovskite for a thick HTL. Thus, spiro-MeOTAD is a very good HTL choice from the device physics' point of view. The fill factor analyzed by the Suns-V-oc method is not transport limited, but trap-recombination limited as well. Consequently, a further optimization of the device has to focus on defects in the polycrystalline perovskite film.
引用
收藏
页码:4200 / 4209
页数:10
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