Accelerated Degradation of FAPbI3 Perovskite by Excess Charge Carriers and Humidity
Excess charge carriers in metal halide perovskite layer have been known to accelerate degradation of the film and devices to cause poor operational stability of perovskite solar cells (PSCs). While mechanisms for such degradation have been predominantly studied for methylammonium‐based perovskites,...
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Veröffentlicht in: | Solar RRL 2024-03, Vol.8 (5), p.n/a |
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Sprache: | eng |
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Zusammenfassung: | Excess charge carriers in metal halide perovskite layer have been known to accelerate degradation of the film and devices to cause poor operational stability of perovskite solar cells (PSCs). While mechanisms for such degradation have been predominantly studied for methylammonium‐based perovskites, effects of excess charge carriers and their interplays with other degradation causes are barely studied for widely used formamidinium‐based perovskites. Herein, a possible decomposition mechanism of the formamidinium lead tri‐iodide (FAPbI3) perovskite in the presence of excess charge under different humidity levels is investigated. The operating condition with excessive charges is simulated by placing half devices with either electron‐transporting layer (ETL) or hole‐transporting layer (HTL) under 1 sun illumination. FAPbI3 in contact with ETL degrades more rapidly than the one with HTL, which is attributed to excess hole charge carriers in the film. Under higher humidity, the synergetic effect of excess charge carriers and humidity is found and thus degradation pathway and kinetics are strongly dependent on the humidity level. The fundamental understanding of degradation pathways for formamidinium perovskites should provide a useful insight toward the development of efficient and operationally stable PSCs toward practical usage.
The excess hole charge carriers in the FAPbI3 film accelerate degradation of the film under ambient atmosphere. The degradation route differs depending on the ambient humidity levels: amorphization occurs under relative humidity (RH) 5 ± 3%, hydrate species are formed under RH 35 ± 3%, and phase changes to nonperovskite δ‐FAPbI3 under RH 45%±3%. |
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ISSN: | 2367-198X 2367-198X |
DOI: | 10.1002/solr.202300958 |