Understanding the Anomalous J-V Curves in Carbon-Based Perovskite Solar Cells as a Structural Transition Induced by Ion Diffusion

被引:7
作者
De Moor, Gilles [1 ]
Charvin, Nicolas [1 ]
Farha, Cynthia [1 ]
Meyer, Toby [2 ]
Perrin, Lara [1 ]
Planes, Emilie [1 ]
Flandin, Lionel [1 ]
机构
[1] Univ Grenoble Alpes, Univ Savoie Mt Blanc, CNRS, Grenoble INP,LEPMI, F-38000 Grenoble, France
[2] Solaronix SA, Rue Ouriette 129, CH-1170 Aubonne, Switzerland
关键词
activation energies; characteristic times; hysteresis; ion migrations; perovskites; structural transitions; ACTIVATION-ENERGY; HYSTERESIS; DIODE; MODEL; PERFORMANCE; EFFICIENCY; TRANSPORT;
D O I
10.1002/solr.202300998
中图分类号
TE [石油、天然气工业]; TK [能源与动力工程];
学科分类号
0807 ; 0820 ;
摘要
The investigation of hole transport layer-free mesoporous carbon perovskite solar cells by analyzing current-voltage (J-V) curves under different scan rates, light intensities, and temperatures is presented. A distinctive bump in the curves is identified, previously reported in the literature. The voltage at the inflection point of this transition shows a linear correlation with the scan rate, directly yielding a characteristic relaxation time. Increasing temperature demonstrates a reduction in the magnitude and characteristic time of the bump. It also indicates an activation energy of 0.8 eV, suggesting a diffusion mechanism. Importantly, the intensity of the illumination has no influence on the overall behavior, indicating that the phenomenon is not a photovoltaic processes. It is proposed that the bump originates from transition between a metastable state at high scan rates and a stable one reached after relaxation. To accurately replicate the measured J-V curves, a novel lumped circuit model is introduced and validated. A schematic microstructural model depicts the reversible reduction in photocurrent as a decline in charge transfer capacity caused by the diffusion of large ions at the mesoporous titanuim dioxyde interface. Ultimately, this study also suggests a plausible reason for the well-known hysteresis commonly observed with perovskite solar cells.
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页数:13
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