Charge carrier transport in polycrystalline CH3NH3PbI3 perovskite thin films in a lateral direction characterized by time-of-flight photoconductivity

被引:11
作者
Emin, S. [1 ]
Pavlica, E. [2 ]
Okuyucu, H. [3 ]
Valant, M. [1 ,4 ]
Bratina, G. [2 ]
机构
[1] Univ Nova Gorica, Mat Res Lab, Vipavska 13, SI-5000 Nova Gorica, Slovenia
[2] Univ Nova Gorica, Lab Organ Matter Phys, Vipavska 13, SI-5000 Nova Gorica, Slovenia
[3] Yildirim Beyazit Univ, Fac Engn, Ankara, Turkey
[4] Univ Elect Sci & Technol China, Inst Fundamental & Frontier Sci, Chengdu 610054, Sichuan, Peoples R China
关键词
CH3NH3PbI3; Time-of-flight photoconductivity; Monte Carlo simulation; Carrier mobility; SOLAR-CELLS; DIFFUSION; RECOMBINATION; MOBILITIES; EFFICIENT; PLANAR; DEGRADATION; MICROMETER; LIFETIMES; MIGRATION;
D O I
10.1016/j.matchemphys.2018.08.012
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
We used time-of-flight photocurrent measurements to determine the role of grain boundaries in charge carrier transport in thin layers of methyl ammonium lead iodide (CH3NH3PbI3). The measurement results were compared to Kinetic Monte Carlo simulations, based on a transport model, which disentangles the transport within crystallites and hopping across grain boundaries. The observed mobilities of electrons are in the order similar to 2.5 x 10(-1) cm(2) V- 1 s(-1) . The hopping across grains is modeled with an Arrhenius-type probability rate, characterized by activation energy (E-a). It was found that the E-a estimated from the slope of a mobility-temperature dependence is in the range of similar to 56-70 meV. The factors contributing to E-a are shunting pathways and the grain-size variations including energy level misalignments at the grain boundaries. These results represent a step toward a design of novel windowless organic-inorganic perovskite solar cells.
引用
收藏
页码:182 / 189
页数:8
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