Abstract:Herein,
we report the nanoscale visualization of the photochemical
degradation dynamics of MAPbI3 (MA = CH3NH3
+) using infrared scattering scanning near-field
microscopy (IR s-SNOM) combined with a series of complementary analytical
techniques such as UV–vis and FTIR-spectroscopy, XRD, and XPS.
Light exposure of the MAPbI3 films resulted in a gradual
loss of MA+ cations starting from the grain boundaries
at the film surface and slowly progressing toward the center of the
grains and deeper into the bulk perovs… Show more
“…It is notable that all four perovskites show a substantial increase in PL intensity after exposure to the highest doses of γ rays (5–10 MGy), which resembles the light-induced degradation of perovskite films studied recently . We believe that the PL enhancement is associated with the phase segregation of the aging products from the pristine perovskite phase.…”
supporting
confidence: 60%
“…All perovskite films revealed complex PL dynamics upon exposure to γ rays (Figure B,C). Both MAPbI 3 and FAPbI 3 show steady increases in PL intensity upon exposure to relatively low doses of γ rays of <100 kGy, which could be explained by the radiation-induced material recrystallization similar to what was observed under visible light illumination. , Indeed, such recrystallization should result in a decrease in the density of defects leading to the nonradiative recombination of charge carriers. On the contrary, the PL intensity of mixed-cation (CsFA)PbI 3 and (CsMAFA)PbI 3 perovskite films decayed rapidly upon exposure to even the smallest doses of γ rays (10–50 kGy).…”
mentioning
confidence: 64%
“…We have shown recently that infrared scattering-type scanning near-field optical microscopy (IR s-SNOM) is a powerful technique for studying the light-induced degradation of perovskite films with a nanoscale spatial resolution . Herein, we applied this technique to monitor the radiation-induced degradation of perovskite films deposited on plastic (PET) substrates.…”
Herein, we show that thin films of MAPbI 3 , FAPbI 3 , (CsMA)PbI 3 , and (CsMAFA)PbI 3 , where MA and FA are methylammonium and formamidinium cations, respectively, tolerate ultrahigh doses of γ rays approaching 10 MGy without significant changes in their absorption spectra. However, among the studied materials, FAPbI 3 was the only one that did not form metallic lead due to its extreme radiation hardness. Infrared nearfield optical microscopy revealed the radiation-induced depletion of organic cations from the grains of MAPbI 3 and their accumulation at the grain boundaries, whereas FAPbI 3 on the contrary lost FA cations from the grain boundaries. The multication (CsMAFA)PbI 3 perovskite underwent a facile phase segregation to domains enriched with MA and FA cations, which is a principally new radiation-induced degradation pathway. Our findings suggest that the radiation hardness of the rationally designed perovskite semiconductors could go far beyond the impressive threshold of 10 MGy we set herein for FAPbI 3 films, which opens many exciting opportunities for practical implementation of these materials.
“…It is notable that all four perovskites show a substantial increase in PL intensity after exposure to the highest doses of γ rays (5–10 MGy), which resembles the light-induced degradation of perovskite films studied recently . We believe that the PL enhancement is associated with the phase segregation of the aging products from the pristine perovskite phase.…”
supporting
confidence: 60%
“…All perovskite films revealed complex PL dynamics upon exposure to γ rays (Figure B,C). Both MAPbI 3 and FAPbI 3 show steady increases in PL intensity upon exposure to relatively low doses of γ rays of <100 kGy, which could be explained by the radiation-induced material recrystallization similar to what was observed under visible light illumination. , Indeed, such recrystallization should result in a decrease in the density of defects leading to the nonradiative recombination of charge carriers. On the contrary, the PL intensity of mixed-cation (CsFA)PbI 3 and (CsMAFA)PbI 3 perovskite films decayed rapidly upon exposure to even the smallest doses of γ rays (10–50 kGy).…”
mentioning
confidence: 64%
“…We have shown recently that infrared scattering-type scanning near-field optical microscopy (IR s-SNOM) is a powerful technique for studying the light-induced degradation of perovskite films with a nanoscale spatial resolution . Herein, we applied this technique to monitor the radiation-induced degradation of perovskite films deposited on plastic (PET) substrates.…”
Herein, we show that thin films of MAPbI 3 , FAPbI 3 , (CsMA)PbI 3 , and (CsMAFA)PbI 3 , where MA and FA are methylammonium and formamidinium cations, respectively, tolerate ultrahigh doses of γ rays approaching 10 MGy without significant changes in their absorption spectra. However, among the studied materials, FAPbI 3 was the only one that did not form metallic lead due to its extreme radiation hardness. Infrared nearfield optical microscopy revealed the radiation-induced depletion of organic cations from the grains of MAPbI 3 and their accumulation at the grain boundaries, whereas FAPbI 3 on the contrary lost FA cations from the grain boundaries. The multication (CsMAFA)PbI 3 perovskite underwent a facile phase segregation to domains enriched with MA and FA cations, which is a principally new radiation-induced degradation pathway. Our findings suggest that the radiation hardness of the rationally designed perovskite semiconductors could go far beyond the impressive threshold of 10 MGy we set herein for FAPbI 3 films, which opens many exciting opportunities for practical implementation of these materials.
“…The images were collected using IR s-SNOM in pseudoheterodyne (PsHet) mode using a NeaSpec neaSNOM instrument as described previously. 21,22 The measurements were performed at the vibration frequencies of HTMs (PTAA: 1319, P1: 1266, P2 and P3: 1268 cm À1 ), which do not overlap with the IR frequencies of the MA + cation in perovskite (962 and 1249 cm À1 , Fig. S13, ESI †).…”
Efficient and economic oxidative polymerization enables the synthesis of polytriarylamines (PTAAs), which show comparable performances to high-cost commercial PTAAs in perovskite solar cells delivering efficiencies of 18–20%.
“…A first comprehensive level stems from ex situ and/or post-mortem analysis that allow comparative observations between two different ageing points; being morphological, optical or structural. [13,[39][40] In complementary to this approach, in situ or operando techniques contribute to directly look into the degradation pathways without external manipulation of the material for analysis, or, start and stop in the ageing which may bring unwished effect given the potential perovskite selfhealing properties. [41,42] With this regard, different studies were carried out either on MAPbI 3 or on mixed-cation perovskites using operando transmission electron microscopy (TEM), in situ X-ray diffraction (XRD) or by absorption spectroscopy under different stressors.…”
Hybrid halide perovskite has established its credibility as high performance thin film photovoltaic technology. Perovskite based on formamidinium cation is at the core composition to top performances and stability. Herein, a depth study based on temperature‐controlled in situ X‐ray diffraction focusing on the photo‐active formamidinium lead iodide (α‐FAPbI3) is reported. In particular, the thermal stability of the latter and the degradation pathways under different experimental conditions are clarified. Based on this in situ technique, the lattice thermal expansion coefficient is reported that provides relevant information on possible mechanical stress created upon temperature cycling or damp heat test. The results support that α‐FAPbI3 degradation is substantially accelerated when temperature is combined to illumination and when it is interfaced with the extraction layers. In addition, by contrast to in darkness for which α‐FAPbI3 degrades directly into PbI2, the existence of a temperature gap under illumination involving an intermediate step with a non‐crystalline phase resulting from the perovskite degradation and contributing to the formation of PbI2 by‐product is revealed.
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