Seed‐Assisted Growth of Tin Oxide Transport Layer for Efficient Perovskite Solar Cells
Source abstract
Abstract
Tin oxide has been the mainstream as the electron transport layer for highly efficient perovskite solar cells due to advantages such as high mobility, high transmittance, and strong UV stability. Realizing high‐quality SnO2 layer at low temperature can widen the range of potential applications on both rigid and flexible substrates. Herein, a seed‐assisted growth strategy is developed for the preparation of SnO2 layer at low temperature (100 °C) and the seeds in precursor solution provide preferential nucleation sites. The SnO2 layer via seed‐assisted growth exhibits higher conductivity and mobility which are more than twice those of control samples because of enhanced crystallinity. The resulting solar cells show high Voc of 1.189 V, contributing to a high power conversion efficiency of 25.26%. To current knowledge, this is the highest efficiency for perovskite solar cells with SnO2 layer formed at low temperature (≤100 °C). Contributed by the high‐quality SnO2 layer prepared at low temperature, a high power conversion efficiency over 22% for flexible perovskite solar cells is also achieved.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Chalcogenide Semiconductor Thin Films · Quantum Dots Synthesis And Properties
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
State Key Laboratory of Metal Matrix Composites Shanghai Jiao Tong University Shanghai 200240 China
College of Arts and Sciences University of Tokyo Tokyo 153-8902 Japan
Funding
National Key Research and Development Program of China · National Natural Science Foundation of China
References (43)
Show source-provided references
1. 10.1002/pip.350610.1002/pip.3506 ↗
2. 10.1021/ja809598r10.1021/ja809598r ↗
3. 10.1126/science.122860410.1126/science.1228604 ↗
4. 10.1038/nature1234010.1038/nature12340 ↗
5. 10.1038/nmat401410.1038/nmat4014 ↗
6. 10.1126/science.aad101510.1126/science.aad1015 ↗
7. 10.1038/nature1413310.1038/nature14133 ↗
8. 10.3390/coatings1007069210.3390/coatings10070692 ↗
9. 10.1039/C6TA04503K10.1039/C6TA04503K ↗
10. 10.1016/j.nanoen.2017.08.04110.1016/j.nanoen.2017.08.041 ↗
11. 10.1002/adfm.20210394910.1002/adfm.202103949 ↗
12. 10.1021/acs.chemrev.9b0048310.1021/acs.chemrev.9b00483 ↗
13. 10.1038/s41586-021-03964-810.1038/s41586-021-03964-8 ↗
14. 10.1038/s41586-021-03285-w10.1038/s41586-021-03285-w ↗
15. 10.1002/adfm.20200155910.1002/adfm.202001559 ↗
16. 10.1021/jacs.5b0199410.1021/jacs.5b01994 ↗
17. 10.1021/jacs.0c0222710.1021/jacs.0c02227 ↗
18. 10.1002/adma.20210987910.1002/adma.202109879 ↗
19. 10.1002/adma.20220168110.1002/adma.202201681 ↗
20. 10.1039/D1EE01519B10.1039/D1EE01519B ↗
21. 10.1002/adma.20210553910.1002/adma.202105539 ↗
22. 10.1016/j.joule.2021.04.01410.1016/j.joule.2021.04.014 ↗
23. 10.1002/aenm.20190348710.1002/aenm.201903487 ↗
24. 10.1002/adfm.20190055710.1002/adfm.201900557 ↗
25. 10.1021/acsami.1c1322210.1021/acsami.1c13222 ↗
26. 10.1021/acsenergylett.8b0069210.1021/acsenergylett.8b00692 ↗
27. 10.1002/adfm.20180866710.1002/adfm.201808667 ↗
28. 10.1002/adma.20170482510.1002/adma.201704825 ↗
29. 10.1002/pip.348710.1002/pip.3487 ↗
30. 10.1002/aenm.20190083410.1002/aenm.201900834 ↗
31. 10.1016/j.joule.2022.12.00610.1016/j.joule.2022.12.006 ↗
32. 10.1038/s41566-019-0398-210.1038/s41566-019-0398-2 ↗
33. 10.1038/s41586-022-04604-510.1038/s41586-022-04604-5 ↗
34. 10.1002/adma.20220472610.1002/adma.202204726 ↗
35. 10.1002/anie.20160473110.1002/anie.201604731 ↗
36. 10.1016/j.joule.2019.03.02310.1016/j.joule.2019.03.023 ↗
37. 10.1038/s41467-018-04029-710.1038/s41467-018-04029-7 ↗
38. 10.1002/smll.20200153510.1002/smll.202001535 ↗
39. 10.1016/S0022-0248(99)00202-X10.1016/S0022-0248(99)00202-X ↗
40. 10.1038/s41586-019-1036-310.1038/s41586-019-1036-3 ↗
41. 10.1126/science.abh388410.1126/science.abh3884 ↗
42. Liu J. · Angew. Chem. Int. Ed. Engl. · 2022 · 10 · 202202012
43. 10.1039/C5EE03229F10.1039/C5EE03229F ↗