Performance Enhancement of Lead-Free Tin-Based Perovskite Solar Cells with Reducing Atmosphere-Assisted Dispersible Additive
Source abstract
Abstract
Sn-based halide perovskite materials have attracted tremendous attention and have been employed successfully in solar cells. However, their high conductivities resulting from the unstable divalent Sn state in the structure cause poor device performance and poor reproducibility. Herein, we used excess tin iodide (SnI 2 ) in Sn-based halide perovskite solar cells (ASnI 3, A = Cs, methylammonium, and formamidinium tin iodide as the representative light absorbers) combined with a reducing atmosphere to stabilize the Sn 2+ state. Excess SnI 2 can disperse uniformly into the perovskite films and functions as a compensator as well as a suppressor of Sn 2+ vacancies, thereby effectively reducing the p-type conductivity. This process significantly improved the solar cell performances of all the ASnI 3 materials on mesoporous TiO 2 . Optimized CsSnI 3 devices achieved a maximum power conversion efficiency of 4.81%, which is the highest among all inorganic Pb-free perovskite solar cells to date.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Conducting polymers and applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Chemistry, Northwestern University, 2145 Sheridan Road, Evanston, Illinois 60208, United States
Mitsubishi Chemical Group Science & Technology Research Center, Inc., 1000 Kamoshida-cho, Aoba-ku, Yokohama 227-8502, Japan
References (43)
Show source-provided references
1. 10.1038/nmat427110.1038/nmat4271 ↗
2. 10.1038/ncomms640410.1038/ncomms6404 ↗
3. 10.1021/acs.accounts.5b0022910.1021/acs.accounts.5b00229 ↗
4. 10.1002/adma.20160026510.1002/adma.201600265 ↗
5. 10.1126/science.aaa927210.1126/science.aaa9272 ↗
6. 10.1038/nenergy.2015.1710.1038/nenergy.2015.17 ↗
7. 10.1126/science.124398210.1126/science.1243982 ↗
8. 10.1021/jz500279b10.1021/jz500279b ↗
9. 10.1021/acs.jpclett.5b0050410.1021/acs.jpclett.5b00504 ↗
10. 10.1021/acs.jpclett.6b0011810.1021/acs.jpclett.6b00118 ↗
11. 10.1021/jacs.5b0102510.1021/jacs.5b01025 ↗
12. 10.1039/C5TA05741H10.1039/C5TA05741H ↗
13. 10.1021/acsenergylett.6b0047110.1021/acsenergylett.6b00471 ↗
14. 10.1021/acs.jpclett.6b0268210.1021/acs.jpclett.6b02682 ↗
15. 10.1021/acs.chemmater.5b0198910.1021/acs.chemmater.5b01989 ↗
16. 10.1021/acsenergylett.6b0049910.1021/acsenergylett.6b00499 ↗
17. 10.1038/nphoton.2014.8210.1038/nphoton.2014.82 ↗
18. 10.1021/ic401215x10.1021/ic401215x ↗
19. 10.1039/C4EE01076K10.1039/C4EE01076K ↗
20. 10.1002/adma.20160299210.1002/adma.201602992 ↗
21. 10.1021/ja301539s10.1021/ja301539s ↗
22. 10.1016/j.jssc.2013.07.00810.1016/j.jssc.2013.07.008 ↗
23. 10.1039/c0dt01601b10.1039/c0dt01601b ↗
24. 10.1063/1.496146310.1063/1.4961463 ↗
25. 10.1021/jz500211710.1021/jz5002117 ↗
26. 10.1002/adma.20140164110.1002/adma.201401641 ↗
27. 10.1002/adfm.20150512710.1002/adfm.201505127 ↗
28. 10.1021/jacs.6b0014210.1021/jacs.6b00142 ↗
29. 10.1002/adma.20140199110.1002/adma.201401991 ↗
30. 10.1021/jp512662410.1021/jp5126624 ↗
31. 10.1039/C5TA00190K10.1039/C5TA00190K ↗
32. 10.1038/nature1106710.1038/nature11067 ↗
33. 10.1021/cm503122j10.1021/cm503122j ↗
34. 10.1021/acsenergylett.6b0051310.1021/acsenergylett.6b00513 ↗
35. 10.1021/jacs.6b1073410.1021/jacs.6b10734 ↗
36. 10.1002/aenm.20160113010.1002/aenm.201601130 ↗
37. 10.1039/C5TA06398A10.1039/C5TA06398A ↗
38. 10.1021/acs.jpclett.6b0157610.1021/acs.jpclett.6b01576 ↗
39. 10.1039/C5TA02950C10.1039/C5TA02950C ↗
40. 10.1021/jacs.6b0879010.1021/jacs.6b08790 ↗
41. 10.1021/ja903481810.1021/ja9034818 ↗
42. 10.1063/1.490518010.1063/1.4905180 ↗
43. 10.1063/1.113644810.1063/1.1136448 ↗