Abstract
CsPbI3 is a promising material for optoelectronics owing to its thermal robustness and favorable bandgap. However, its fabrication is challenging because its photoactive phase is thermodynamically unstable at room temperature. Adding dimethylammonium (DMA) alleviates this instability and is currently understood to result in the formation of DMAxCs1–xPbI3 perovskite solid solutions. Here, we use NMR of the 133Cs and 13C local structural probes to show that these solid solutions are not thermodynamically stable, and their synthesis under thermodynamic control leads to a segregated mixture of yellow one-dimensional DMAPbI3 phase and δ-CsPbI3. We show that mixed-cation DMAxCs1–xPbI3 perovskite phases only form when they are kinetically trapped by rapid antisolvent-induced crystallization. We explore the energetics of DMA incorporation into CsPbI3 using first-principles calculations and molecular dynamics simulations and find that this process is energetically unfavorable. Our results provide a complete atomic-level picture of the mechanism of DMA-induced stabilization of the black perovskite phase of CsPbI3 and shed new light on this deceptively simple material.
Original language | English |
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Pages (from-to) | 2745–2752 |
Number of pages | 8 |
Journal | ACS Energy Letters |
Volume | 7 |
Issue number | 8 |
Early online date | 26 Jul 2022 |
DOIs | |
Publication status | Published - 12 Aug 2022 |
Bibliographical note
Acknowledgments:We thank Zaiwei Wang for discussions and help in designing preliminary experiments. D.J.K. acknowledges the support of the University of Warwick. A.M. and L.E. are grateful for the support from SNSF grant number 200020_178860, and U.R. acknowledges funding from SNSF grant number 200020-185092 and the NCCR MUST. Computing time was provided by the Swiss National Computing Centre CSCS. R.D.C and D.P. acknowledge the National Science Centre (Grant SONATA BIS 10, No. 2020/38/E/ST5/00267) for financial support.