4.8 Article

High grain boundary recombination velocity in polycrystalline metal halide perovskites

Journal

SCIENCE ADVANCES
Volume 8, Issue 36, Pages -

Publisher

AMER ASSOC ADVANCEMENT SCIENCE
DOI: 10.1126/sciadv.abq8345

Keywords

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Funding

  1. Center for Hybrid Organic Inorganic Semiconductors for Energy (CHOISE), an Energy Frontier Research Center - Office of Basic Energy Sciences, Office of Science within the U.S. Department of Energy
  2. Defense Threat Reduction Agency [HDTRA1-20-2-0002]
  3. National Science Foundation [DMR-1903981]
  4. U.S. Department of Energy's Office of Energy Efficiency and Renewable Energy (EERE) under Solar Energy Technologies Office (SETO) [DE-EE0009520]

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This study reports the determination of carrier recombination velocities at grain boundaries of polycrystalline perovskites through mapping transient photoluminescence pattern changes. It reveals that charge recombination at grain boundaries is stronger than at surfaces, and introduces a surface treatment method to reduce the recombination velocity, enhancing the efficiency of perovskite solar cells.
Understanding carrier recombination processes in metal halide perovskites is fundamentally important to further improving the efficiency of perovskite solar cells, yet the accurate recombination velocity at grain boundaries (GBs) has not been determined. Here, we report the determination of carrier recombination velocities at GBs (S-GB) of polycrystalline perovskites by mapping the transient photoluminescence pattern change induced by the nonradiative recombination of carriers at GBs. Charge recombination at GBs is revealed to be even stronger than at surfaces of unpassivated films, with average S-GB reaching 2200 to 3300 cm/s. Regular surface treatments do not passivate GBs because of the absence of contact at GBs. We find a surface treatment using tributyl(methyl)phosphonium dimethyl phosphate that can penetrate into GBs by partially dissolving GBs and converting it into one-dimensional perovskites. It reduces the average S-GB by four times, with the lowest S-GB of 410 cm/s, which is comparable to surface recombination velocities after passivation.

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