Abstract
Coevaporation of formamidinium lead iodide (FAPbI3) is a promising route for the fabrication of highly efficient and scalable optoelectronic devices, such as perovskite solar cells. However, it poses experimental challenges in achieving stoichiometric FAPbI3 films with a cubic structure (α-FAPbI3). In this work, we show that undesired hexagonal phases of both PbI2 and FAPbI3 form during thermal evaporation, including the well-known 2H-FAPbI3, which are detrimental for optoelectronic performance. We demonstrate the growth of α-FAPbI3 at room temperature via thermal evaporation by depositing phosphonic acids (PAc) on substrates and subsequently coevaporating PbI2 and formamidinium iodide. We use density-functional theory to develop a theoretical model to understand the relative growth energetics of the α and 2H phases of FAPbI3 for different molecular interactions. Experiments and theory show that the presence of PAc molecules stabilizes the formation of α-FAPbI3 in thin films when excess molecules are available to migrate during growth. This migration of molecules facilitates the continued presence of adsorbed organic precursors at the free surface throughout the evaporation, which lowers the growth energy of the α-FAPbI3 phase. Our theoretical analyses of PAc molecule-molecule interactions show that ligands can form hydrogen bonding to reduce the migration rate of the molecules through the deposited film, limiting the effects on the crystal structure stabilization. Our results also show that the phase stabilization with molecules that migrate is long-lasting and resistant to moist air. These findings enable reliable formation and processing of α-FAPbI3 films via vapor deposition.
Original language | English |
---|---|
Pages (from-to) | 18459-18469 |
Number of pages | 11 |
Journal | Journal of the American Chemical Society |
Volume | 146 |
Issue number | 27 |
DOIs | |
State | Published - Jul 10 2024 |
Funding
The work by J.-P. C.-B. and A.-F. C.-M. (experimental), and F. J. and A. M. R. (theoretical and computational modeling) was supported by the National Science Foundation, Science and Technology Center Program (IMOD), under grant no. DMR-2019444. This work was performed in part at the Georgia Tech Institute for Electronics and Nanotechnology, a member of the National Nanotechnology Coordinated Infrastructure (NNCI), which is supported by the National Science Foundation (Grant ECCS-1542174). A.-F.C.-M. received funding from the Colombian Ministry of Sciences and Technology and the U.S. Department of State under a Fulbright Scholarship. This research used CMS beamline of the National Synchrotron Light Source II, a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Brookhaven National Laboratory under contract no. DE-SC0012704. Computational support was provided by the National Energy Research Scientific Computing Center (NERSC), a US Department of Energy, Office of Science User Facility, located at Lawrence Berkeley National Laboratory, operated under contract no. DE-AC02-05CH11231. We thank Dr. Juanita Hidalgo for the discussions related to the structural characterization. Cathodoluminescence SEM microscopy was performed at the Center for Nanophase Materials Sciences (CNMS), which is a U.S. Department of Energy Office of Science User Facility at Oak Ridge National Laboratory under proposal CNMS2023-A-01935. D.K.L. was funded by a National Science Foundation Graduate Research Fellowship Program under grant no. DGE-2039655. C.A.R.P. and J.-P.C.-B. acknowledge the support of the National Aeronautics and Space Administration (award no. 80NSSC19M0201). Any opinions, findings, and conclusions or recommendations expressed in this material are those of the authors(s) and do not necessarily reflect the views of the National Science Foundation.