Magnetic Field-Assisted Perovskite Film Preparation for Enhanced Performance of Solar Cells
Source abstract
Abstract
Perovskite solar cells (PSCs) are promising low-cost photovoltaic technologies with high power conversion efficiency (PCE). The crystalline quality of perovskite materials is crucial to the photovoltaic performance of the PSCs. Herein, a simple approach is introduced to prepare high-quality CH 3 NH 3 PbI 3 perovskite films with larger crystalline grains and longer carriers lifetime by using magnetic field to control the nucleation and crystal growth. The fabricated planar CH 3 NH 3 PbI 3 solar cells have an average PCE of 17.84% and the highest PCE of 18.56% using an optimized magnetic field at 80 mT. In contrast, the PSCs fabricated without the magnetic field give an average PCE of 15.52% and the highest PCE of 16.72%. The magnetic field action produces an ordered arrangement of the perovskite ions, improving the crystallinity of the perovskite films and resulting in a higher PCE.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Solid-state spectroscopy and crystallography
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Dalian Institute of Chemical Physics, Dalian National Laboratory for Clean Energy, Chinese Academy of Sciences, Dalian 116023, China
Funding
Ministry of Science and Technology of the People's Republic of China · China Postdoctoral Science Foundation · National Natural Science Foundation of China · Central Committee of the Communist Party of China · National University Research Fund, China
References (45)
Show source-provided references
1. 10.1021/ja809598r10.1021/ja809598r ↗
2. 10.1126/science.122860410.1126/science.1228604 ↗
3. 10.1038/nature1250910.1038/nature12509 ↗
4. 10.1126/science.125405010.1126/science.1254050 ↗
5. National Renewable Energy Laboratory, Best Research-Cell Efficiencies chart.www.nrel.gov/ncpv/images/efficiency_chart.jpg.
6. 10.1038/nenergy.2016.14810.1038/nenergy.2016.148 ↗
7. 10.1002/aenm.20160046010.1002/aenm.201600460 ↗
8. 10.1039/C5TA09249C10.1039/C5TA09249C ↗
9. 10.1063/1.494123810.1063/1.4941238 ↗
10. 10.1039/C5TA01824B10.1039/C5TA01824B ↗
11. 10.1002/aenm.20140122910.1002/aenm.201401229 ↗
12. 10.1002/adma.20140537210.1002/adma.201405372 ↗
13. 10.1126/science.125476310.1126/science.1254763 ↗
14. 10.1038/ncomms678410.1038/ncomms6784 ↗
15. 10.1038/nmat401410.1038/nmat4014 ↗
16. 10.1021/acsami.6b1263710.1021/acsami.6b12637 ↗
17. 10.1002/aenm.20160076710.1002/aenm.201600767 ↗
18. 10.1021/acsami.6b0878310.1021/acsami.6b08783 ↗
19. 10.1002/aenm.20150208710.1002/aenm.201502087 ↗
20. 10.1021/acsami.6b0684710.1021/acsami.6b06847 ↗
21. 10.1021/acsami.5b1149410.1021/acsami.5b11494 ↗
22. 10.1021/ja411509g10.1021/ja411509g ↗
23. 10.1126/science.aaa047210.1126/science.aaa0472 ↗
24. 10.1126/science.aaf806010.1126/science.aaf8060 ↗
25. 10.1038/nenergy.2016.14210.1038/nenergy.2016.142 ↗
26. 10.1021/acsami.6b1556310.1021/acsami.6b15563 ↗
27. 10.1039/C6CC00753H10.1039/C6CC00753H ↗
28. 10.1038/nphys327710.1038/nphys3277 ↗
29. 10.1002/adma.20140177510.1002/adma.201401775 ↗
30. 10.1038/ncomms1110510.1038/ncomms11105 ↗
31. 10.1126/science.aaa533310.1126/science.aaa5333 ↗
32. 10.1021/ja512833n10.1021/ja512833n ↗
33. 10.1039/C5EE02155C10.1039/C5EE02155C ↗
34. 10.1002/adma.20160044610.1002/adma.201600446 ↗
35. 10.1126/science.aad181810.1126/science.aad1818 ↗
36. 10.1063/1.490151010.1063/1.4901510 ↗
37. 10.1126/science.aaa272510.1126/science.aaa2725 ↗
38. 10.1002/adma.20150258610.1002/adma.201502586 ↗
39. 10.1002/aenm.20150180310.1002/aenm.201501803 ↗
40. 10.1016/j.jcrysgro.2006.11.34510.1016/j.jcrysgro.2006.11.345 ↗
41. 10.1016/j.jcrysgro.2011.11.08010.1016/j.jcrysgro.2011.11.080 ↗
42. 10.1016/j.jcrysgro.2013.01.01710.1016/j.jcrysgro.2013.01.017 ↗
43. 10.1016/j.jcrysgro.2015.07.03410.1016/j.jcrysgro.2015.07.034 ↗
44. 10.1038/ncomms1155510.1038/ncomms11555 ↗
45. 10.1002/adma.20150414410.1002/adma.201504144 ↗