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

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 ∼2.5 × 10⁻¹ cm²V⁻¹s⁻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 ∼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.