1.State Key Laboratory of Physical Chemistry of Solid Surfaces, Collaborative Innovation Center of Chemistry for Energy Materials, College of Chemistry and Chemical Engineering, Xiamen University, Xiamen, China
2.School of Aerospace Engineering, Xiamen University, Xiamen, China
Song-Yuan Ding (syding@xmu.edu.cn)
Bing-Wei Mao (bwmao@xmu.edu.cn)
纸质出版日期:2021-05-31,
网络出版日期:2021-04-15,
收稿日期:2020-11-10,
修回日期:2021-03-24,
录用日期:2021-03-29
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Quantification of electron accumulation at grain boundaries in perovskite polycrystalline films by correlative infrared-spectroscopic nanoimaging and Kelvin probe force microscopy[J]. LSA, 2021,10(5):890-897.
Qin, T. X. et al. Quantification of electron accumulation at grain boundaries in perovskite polycrystalline films by correlative infrared-spectroscopic nanoimaging and Kelvin probe force microscopy. Light: Science & Applications, 10, 890-897 (2021).
Quantification of electron accumulation at grain boundaries in perovskite polycrystalline films by correlative infrared-spectroscopic nanoimaging and Kelvin probe force microscopy[J]. LSA, 2021,10(5):890-897. DOI: 10.1038/s41377-021-00524-7.
Qin, T. X. et al. Quantification of electron accumulation at grain boundaries in perovskite polycrystalline films by correlative infrared-spectroscopic nanoimaging and Kelvin probe force microscopy. Light: Science & Applications, 10, 890-897 (2021). DOI: 10.1038/s41377-021-00524-7.
Organic-inorganic halide perovskites are emerging materials for photovoltaic applications with certified power conversion efficiencies (PCEs) ov
er 25%. Generally
the microstructures of the perovskite materials are critical to the performances of PCEs. However
the role of the nanometer-sized grain boundaries (GBs) that universally existing in polycrystalline perovskite films could be benign or detrimental to solar cell performance
still remains controversial. Thus
nanometer-resolved quantification of charge carrier distribution to elucidate the role of GBs is highly desirable. Here
we employ correlative infrared-spectroscopic nanoimaging by the scattering-type scanning near-field optical microscopy with 20 nm spatial resolution and Kelvin probe force microscopy to quantify the density of electrons accumulated at the GBs in perovskite polycrystalline thin films. It is found that the electron accumulations are enhanced at the GBs and the electron density is increased from 6 × 10
19
cm
−3
in the dark to 8 × 10
19
cm
−3
under 10 min illumination with 532 nm light. Our results reveal that the electron accumulations are enhanced at the GBs especially under light illumination
featuring downward band bending toward the GBs
which would assist in electron-hole separation and thus be benign to the solar cell performance.
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