journal article·2016-07-08

Correlations between Immobilizing Ions and Suppressing Hysteresis in Perovskite Solar Cells

Yicheng Zhao, Wenke Zhou, Wei Ma, Sheng Meng, Heng Li, Jing Wei, Rui Fu, Kaihui Liu, Dapeng Yu, Qing Zhao

ACS Energy Letters· Volume 1· Issue 1
Publisher page

Abstract

Ion migration has been regarded as the major cause of photocurrent hysteresis. Here we use photoluminescence (PL) and optical images, combined with Galvanostatic measurement, to detect the ionic motion. We observe an irreversible PL and optical transmittance change after electric poling. By comparing a neat perovskite film with the sample coated by poly(methyl methacrylate) (PMMA), polyethylene glycol (PEG), and [6,6]-phenyl-C61-butyric acid methyl ester (PCBM), we found that PCBM effectively inhibits ionic motion near the surface of the perovskite.We further evidenced the donor–acceptor complex formed between PCBM and perovskite, implying the mechanism of inhibited ion migration by PCBM. We close by demonstrating that PCBM can also be introduced on the top of perovskite fim in an n–i–p TiO 2 planar structure, to achieve an average 14% steady-state output over 2.3 × 10 5 s (∼64 h). This work highlights the importance of inhibiting ionic motion in perovskite solar cells.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · Conducting polymers and applications · Organic Electronics and Photovoltaics

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

State Key Laboratory for Mesoscopic Physics, School of Physics, Peking University, 100871 Beijing, China

Collaborative Innovation Center of Quantum Matter, 100084 Beijing, China

Institute of Physics, Chinese Academy of Sciences, 100190 Beijing, China

Funding

Program for New Century Excellent Talents in University · Ministry of Science and Technology of the People's Republic of China · National Natural Science Foundation of China · Beijing Nova Program

References (37)

Show source-provided references
1. 10.1038/nature1234010.1038/nature12340 ↗
2. 10.1126/science.122860410.1126/science.1228604 ↗
3. 10.1038/nature1250910.1038/nature12509 ↗
4. 10.1126/science.125405010.1126/science.1254050 ↗
5. 10.1126/science.124398210.1126/science.1243982 ↗
6. 10.1021/jz502111u10.1021/jz502111u ↗
7. 10.1021/nl500390f10.1021/nl500390f ↗
8. 10.1038/nnano.2015.9010.1038/nnano.2015.90 ↗
9. 10.1021/jz500113x10.1021/jz500113x ↗
10. 10.1038/nmat406510.1038/nmat4065 ↗
11. 10.1038/ncomms714210.1038/ncomms7142 ↗
12. 10.1038/ncomms1003010.1038/ncomms10030 ↗
13. 10.1021/jacs.5b0493010.1021/jacs.5b04930 ↗
14. 10.1038/nature1413310.1038/nature14133 ↗
15. 10.1021/nn505723h10.1021/nn505723h ↗
16. 10.1021/nn503647610.1021/nn5036476 ↗
17. 10.1039/C4MH00238E10.1039/C4MH00238E ↗
18. 10.1038/ncomms849710.1038/ncomms8497 ↗
19. 10.1002/anie.20150001410.1002/anie.201500014 ↗
20. 10.1039/C5EE01265A10.1039/C5EE01265A ↗
21. 10.1038/nmat415010.1038/nmat4150 ↗
22. 10.1002/aenm.20150180310.1002/aenm.201501803 ↗
23. 10.1002/aenm.20150096210.1002/aenm.201500962 ↗
24. 10.1021/jacs.5b0908510.1021/jacs.5b09085 ↗
25. 10.1063/1.143316410.1063/1.1433164 ↗
26. 10.1063/1.11979710.1063/1.119797 ↗
27. 10.1143/JPSJ.8.59510.1143/JPSJ.8.595 ↗
28. 10.1143/JPSJ.16.221310.1143/JPSJ.16.2213 ↗
29. 10.1111/j.1151-2916.1990.tb09811.x10.1111/j.1151-2916.1990.tb09811.x ↗
30. 10.1021/ja507930510.1021/ja5079305 ↗
31. 10.1038/ncomms678410.1038/ncomms6784 ↗
32. 10.1039/C4EE01138D10.1039/C4EE01138D ↗
33. 10.1039/C4EE03664F10.1039/C4EE03664F ↗
34. 10.1038/ncomms808110.1038/ncomms8081 ↗
35. 10.1002/adma.20130058010.1002/adma.201300580 ↗
36. 10.1103/PhysRevB.57.758610.1103/PhysRevB.57.7586 ↗
37. 10.1134/S106377450804014710.1134/S1063774508040147 ↗