氧烷
扩展X射线吸收精细结构
卤化物
钙钛矿(结构)
亚稳态
成核
谱线
化学物理
从头算量子化学方法
从头算
吸收光谱法
物理化学
化学
材料科学
结晶学
无机化学
有机化学
分子
物理
量子力学
天文
作者
Nadia N. Intan,Blaire A. Sorenson,Yong Kyu Choi,Joshua J. Choi,John L. Fulton,Niranjan Govind,Shelly D. Kelly,Gregory K. Schenter,Paulette Clancy,Christopher J. Mundy
标识
DOI:10.1021/acs.chemmater.4c01523
摘要
Using complementary experimental measurements and computational predictions of spectroscopic measurements (EXAFS, XANES, and UV–vis), we have determined the identity of the most stable iodoplumbate species in dilute lead halide perovskite precursor solutions. We have determined which species are most likely to be thermodynamically stable compared to others that are unstable or metastable. Condensed phase ab initio models were constructed, and the resulting ensembles were used to directly compare the computed signals to the experimental results of the EXAFS, XANES, and UV–vis spectra of PbI2:MAI in DMF. The results of this study suggest that only Pb2+, PbI+, and PbI2 are dominant in the dilute lead perovskite precursor solutions as thermodynamically stable entities. Our interpretation of the relative stability of iodoplumbate species in solution, based on an analysis of EXAFS and XANES spectra, provides critically important new insight into the species most likely to be responsible for crystal nucleation and growth in these materials. This insight will have a significant consequence on the broad scientific community and will necessitate the reinterpretation of peaks in the UV–vis spectra of lead halide perovskite precursor solutions.
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