Halogen Migration in Hybrid Perovskites: The Organic Cation Matters
KAUST DepartmentChemical Science Program
Functional Nanomaterials Lab (FuNL)
KAUST Catalysis Center (KCC)
KAUST Solar Center (KSC)
Material Science and Engineering Program
Physical Science and Engineering (PSE) Division
Ultrafast Laser Spectroscopy and Four-dimensional Electron Imaging Research Group
Online Publication Date2018-09-06
Print Publication Date2018-09-20
Permanent link to this recordhttp://hdl.handle.net/10754/630525
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AbstractIn hybrid perovskite materials, the organic cations are one of the key structural components used to tune the electronic and optical properties of this promising class of materials. Here, we studied the strong impact of organic cations, methylammonium (MA) and formamidinium (FA), on halogen vacancy and interstitial migration, as well as surface degradation in cubic-phase MAPbBr3 and FAPbBr3 crystals using density functional theory calculations. We found Br vacancies and interstitials have much lower formation energies and higher density in MAPbBr3 in comparison to FAPbBr3 crystals. Moreover, the transition energy barrier for Br migration through vacancies within the bulk phase is lower in MAPbBr3 than in FAPbBr3. We also found that FAPbBr3 has a much higher rotation barrier of the organic cation than MAPbBr3, which points to a much stronger H-bonding with Br in the former case. Our results show that incorporating organic cations with the appropriate structure, shape, and strong H-bonding capabilities in hybrid perovskite crystals is very beneficial for suppressing ion migration and thus further improving the performance of hybrid perovskite-based devices.
CitationOranskaia A, Yin J, Bakr OM, Brédas J-L, Mohammed OF (2018) Halogen Migration in Hybrid Perovskites: The Organic Cation Matters. The Journal of Physical Chemistry Letters 9: 5474–5480. Available: http://dx.doi.org/10.1021/acs.jpclett.8b02522.
SponsorsThis work was supported by the King Abdullah University of Science and Technology (KAUST), the Georgia Research Alliance, and the Vasser-Woolley Foundation. We acknowledge the IT Research Computing Team and Shaheen II KAUST Supercomputer for their computational and storage resources, as well as their gracious assistance.
PublisherAmerican Chemical Society (ACS)