Degradation of Highly Alloyed Metal Halide Perovskite Precursor Inks: Mechanism and Storage Solutions
Source abstract
Abstract
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.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Solid-state spectroscopy and crystallography · Conducting polymers and applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
National Renewable Energy Laboratory, Golden, Colorado 80401, United States
Department of Electrical, Computer and Energy Engineering, University of Colorado Boulder, Boulder, Colorado 80302, United States
Renewable and Sustainable Energy Institute, University of Colorado Boulder, Boulder, Colorado 80309 United States
Funding
U.S. Department of Energy
References (24)
Show source-provided references
1. 10.1021/acs.chemrev.5b0071510.1021/acs.chemrev.5b00715 ↗
2. 10.1039/C6EE03397K10.1039/C6EE03397K ↗
3. 10.1039/C5EE03874J10.1039/C5EE03874J ↗
4. 10.1021/acs.chemmater.5b0410710.1021/acs.chemmater.5b04107 ↗
5. 10.1126/science.aad584510.1126/science.aad5845 ↗
6. 10.1038/nature1413310.1038/nature14133 ↗
7. 10.1126/science.aaf971710.1126/science.aaf9717 ↗
8. 10.1039/C5EE02555A10.1039/C5EE02555A ↗
9. 10.1038/ncomms1407510.1038/ncomms14075 ↗
10. 10.1021/acs.jpclett.7b0212810.1021/acs.jpclett.7b02128 ↗
11. 10.1039/c3ee43822h10.1039/c3ee43822h ↗
12. 10.1039/C5MH00170F10.1039/C5MH00170F ↗
13. 10.1039/C7TC00598A10.1039/C7TC00598A ↗
14. 10.1139/v56-02110.1139/v56-021 ↗
15. 10.1021/jp201864g10.1021/jp201864g ↗
16. 10.1039/C4EE02988G10.1039/C4EE02988G ↗
17. 10.1016/j.joule.2017.09.00910.1016/j.joule.2017.09.009 ↗
18. 10.1021/acs.inorgchem.6b0309510.1021/acs.inorgchem.6b03095 ↗
19. 10.1016/j.jssc.2016.05.01510.1016/j.jssc.2016.05.015 ↗
20. 10.1039/C7TA07413A10.1039/C7TA07413A ↗
21. 10.1557/jmr.2016.27210.1557/jmr.2016.272 ↗
22. Laurence C. · 2010
23. 10.1002/sia.303610.1002/sia.3036 ↗
24. 10.1002/cssc.20160087910.1002/cssc.201600879 ↗