Interpretation of slow electroluminescence and open circuit voltage transient response in Cs-based perovskite solar cells

电致发光 钙钛矿(结构) 材料科学 光电子学 磁滞 载流子 开路电压 太阳能电池 太阳能电池理论 离子 瞬态(计算机编程) 电压 化学 太阳能电池效率 凝聚态物理 纳米技术 物理 图层(电子) 有机化学 量子力学 计算机科学 结晶学 操作系统
作者
Matías Córdoba,Moritz Unmüssig,Jan Herterich,Uli Würfel,K. Taretto
出处
期刊:Journal of Applied Physics [American Institute of Physics]
卷期号:130 (22) 被引量:6
标识
DOI:10.1063/5.0065983
摘要

The desirable small hysteresis in the current–voltage characteristics of perovskite solar cells is often understood as a result of small ionic concentration or mobility and low interface charging by depleted/accumulated ions. However, devices having very small apparent hysteresis at practical scan rates can exhibit strong ionic effects seen in the transient response to excitation events. We explore Cs-based double-cation perovskite solar cells showing vanishing hysteresis and nearly hour-long responses to light- and voltage-step excitation, which are tracked by the evolution of open-circuit voltage and injected current, together with electroluminescence emission, respectively. The observed responses, including the increase of electroluminescence with time, are explained by the modulation of the electric field within the perovskite by mobile ions under the condition of interface recombination of mobile charge carriers dominating overall recombination. This is further explored by a numerical model containing mobile ions, which requires that charge carriers recombine predominantly at the interfaces of the device in order to obtain transient responses comparable to the experiments. Further support for the predominance of interface recombination is experimentally obtained by steady-state photocarrier grating characterization, which yields diffusion lengths of photogenerated carriers above 1 μm, i.e., well above the 300 nm perovskite layer thickness. The numerical model further shows that within the case of dominating interface recombination, the shape of both the light- and voltage-step transient responses are strongly determined by the energy band offsets between the perovskite and the contact layers of the solar cell.
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