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Degradation of Highly Alloyed Metal Halide Perovskite Precursor Inks: Mechanism and Storage Solutions AITranslate

University of Colorado Boulder;National Renewable Energy Laboratory;National Renewable Energy Laboratory;National Renewable Energy Laboratory;National Renewable Energy Laboratory;National Renewable Energy Laboratory; University of Colorado Boulder; University of Colorado Boulder;National Renewable Energy Laboratory
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Publisher: ACS
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Abstract AITranslate

Whereas the promise of metal halide perovskite (MHP) photovoltaics (PV) is that they can combine high efficiency with solution-processability, the chemistry occurring in precursor inks is largely unexplored. Herein, we investigate the degradation of MHP solutions based on the most widely used solvents, dimethylformamide (DMF) and dimethyl sulfoxide (DMSO). For the MHP inks studied, which contain formamidinium (FA+), methylammonium (MA+), cesium (Cs+), lead (Pb2+), bromide (Br–), and iodide (I–), dramatic compositional changes are observed following storage of the inks in nitrogen in the dark. We show that hydrolysis of DMF in the precursor solution forms dimethylammonium formate, which subsequently incorporates into the MHP film to compromise the ability of Cs+ and MA+ to stabilize FA+-based MHP. The changes in solution chemistry lead to a modification of the perovskite film stoichiometry, band gap, and structure. The solid precursor salts are stable when ball-milled into a powder, allowing for the storage of large quantities of stoichiometric precursor materials.

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DOI:https://doi.org/10.1021/acsenergylett.8b00305

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Citation Information:

Whereas the promise of metal halide perovskite (MHP) photovoltaics (PV) is that they can combine high efficiency with solution-processability, the chemistry occurring in precursor inks is largely unexplored. Herein, we investigate the degradation of MHP solutions based on the most widely used solvents, dimethylformamide (DMF) and dimethyl sulfoxide (DMSO). For the MHP inks studied, which contain formamidinium (FA+), methylammonium (MA+), cesium (Cs+), lead (Pb2+), bromide (Br–), and iodide (I–), dramatic compositional changes are observed following storage of the inks in nitrogen in the dark. We show that hydrolysis of DMF in the precursor solution forms dimethylammonium formate, which subsequently incorporates into the MHP film to compromise the ability of Cs+ and MA+ to stabilize FA+-based MHP. The changes in solution chemistry lead to a modification of the perovskite film stoichiometry, band gap, and structure. The solid precursor salts are stable when ball-milled into a powder, allowing for the storage of large quantities of stoichiometric precursor materials.

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GB/T 7714-2015 [1] Benjia Dou, Lance M. Wheeler, Jeffrey A. Christians, et al. ACS Energy Letters, 2018(3). DOI:10.1021/acsenergylett.8b00305.
MLA [1] Benjia Dou, et al., ACS Energy Letters, no. 3, 2018, https://doi.org/10.1021/acsenergylett.8b00305.
APA [1] Benjia Dou, Lance M. Wheeler, Jeffrey A. Christians, David. T. Moore, Steven P. Harvey, Joseph J. Berry, Frank S. Barnes, Sean. E. Shaheen, & Maikel F.A.M. van Hest. (2018). ACS Energy Letters(3). https://doi.org/10.1021/acsenergylett.8b00305
IEEE [1] Benjia Dou, Lance M. Wheeler, Jeffrey A. Christians, David. T. Moore, Steven P. Harvey, Joseph J. Berry, Frank S. Barnes, Sean. E. Shaheen, and Maikel F.A.M. van Hest, ACS Energy Letters, no. 3, 2018, doi: 10.1021/acsenergylett.8b00305.