Gas-solid reaction based over one-micrometer thick stable perovskite films for efficient solar cells and modules

Besides high efficiency, the stability and reproducibility of perovskite solar cells (PSCs) are also key for their commercialization. Herein, we report a simple perovskite formation method to fabricate perovskite films with thickness over 1 μm in ambient condition on the basis of the fast gas−solid...

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Published inNature communications Vol. 9; no. 1; pp. 3880 - 11
Main Authors Liu, Zonghao, Qiu, Longbin, Juarez-Perez, Emilio J., Hawash, Zafer, Kim, Taehoon, Jiang, Yan, Wu, Zhifang, Raga, Sonia R., Ono, Luis K., Liu, Shengzhong (Frank), Qi, Yabing
Format Journal Article
LanguageEnglish
Published London Nature Publishing Group UK 24.09.2018
Nature Publishing Group
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ISSN2041-1723
2041-1723
DOI10.1038/s41467-018-06317-8

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Summary:Besides high efficiency, the stability and reproducibility of perovskite solar cells (PSCs) are also key for their commercialization. Herein, we report a simple perovskite formation method to fabricate perovskite films with thickness over 1 μm in ambient condition on the basis of the fast gas−solid reaction of chlorine-incorporated hydrogen lead triiodide and methylamine gas. The resultant thick and smooth chlorine-incorporated perovskite films exhibit full coverage, improved crystallinity, low surface roughness and low thickness variation. The resultant PSCs achieve an average power conversion efficiency of 19.1 ± 0.4% with good reproducibility. Meanwhile, this method enables an active area efficiency of 15.3% for 5 cm × 5 cm solar modules. The un-encapsulated PSCs exhibit an excellent T 80 lifetime exceeding 1600 h under continuous operation conditions in dry nitrogen environment. Perovskite solar cells often suffer from poor uniformity and reproducibility especially in case of large area devices. Here Liu et al. developed a gas−solid reaction method that enables facile fabrication of over 1 µm thick perovskite films for solar modules with high efficiency, stability and reproducibility.
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ISSN:2041-1723
2041-1723
DOI:10.1038/s41467-018-06317-8