| Literature DB >> 34846843 |
Dohyung Kim1,2, Jihoo Lim3, Seungmin Lee4, Arman Mahboubi Soufiani3, Eunyoung Choi3, Anton V Ievlev5, Nikolay Borodinov5, Yongtao Liu5, Olga S Ovchinnikova6, Mahshid Ahmadi2, Sean Lim7, Pankaj Sharma1, Jan Seidel1, Jun Hong Noh4, Jae Sung Yun3,8.
Abstract
The optoelectronic performance of organic-inorganic halide perovskite (OIHP)-based devices has been improved in recent years. Particularly, solar cells fabricated using mixed-cations and mixed-halides have outperformed their single-cation and single-halide counterparts. Yet, a systematic evaluation of the microstructural behavior of mixed perovskites is missing despite their known composition-dependent photoinstability. Here, we explore microstructural inhomogeneity in (FAPbI3)x(MAPbBr3)1-x using advanced scanning probe microscopy techniques. Contact potential difference (CPD) maps measured by Kelvin probe force microscopy show an increased fraction of grains exhibiting a low CPD with flat topography as MAPbBr3 concentration is increased. The higher portion of low CPD contributes to asymmetric CPD distribution curves. Chemical analysis reveals these grains being rich in MA, Pb, and I. The composition-dependent phase segregation upon illumination, reflected on the emergence of a low-energy peak emission in the original photoluminescence spectra, arises from the formation of such grains with flat topology. Bias-dependent piezo-response force microscopy measurements, in these grains, further confirm vigorous ion migration and cause a hysteretic piezo-response. Our results, therefore, provide insights into the microstructural evaluation of phase segregation and ion migration in OIHPs pointing toward process optimization as a mean to further enhance their optoelectronic performance.Entities:
Keywords: contact potential difference; defects; flat grains; inhomogeneity; ion migration; large bandgap perovskites; phase instability
Year: 2021 PMID: 34846843 DOI: 10.1021/acsnano.1c08726
Source DB: PubMed Journal: ACS Nano ISSN: 1936-0851 Impact factor: 15.881