Transparent Conductive Oxide‐Free Graphene‐Based Perovskite Solar Cells with over 17% Efficiency
Source abstract
Abstract
Highly efficient transparent conductive oxide (TCO)-free perovskite (CH3NH3PbI3) solar cells are demonstrated by using a graphene transparent anode and organic carrier transport materials. By adding a few nanometer-thick MoO3 layer, wettability and work function of the graphene electrode are enhanced to enable a 17.1% power conversion efficiency, which is so far the highest efficiency for TCO-free solar cells. As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re-organized for online delivery, but are not copy-edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors. Please note: The publisher is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Conducting polymers and applications · Chalcogenide Semiconductor Thin Films
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Mechanical and Aerospace Engineering Seoul National University Seoul 08826 South Korea
Global Frontier Center for Multiscale Energy Systems Seoul National University Seoul 08826 South Korea
School of Chemical Engineering and Department of Energy Science Sungkyunkwan University Suwon 16419 South Korea
Funding
National Research Foundation
References (44)
Show source-provided references
1. 10.1021/ja809598r10.1021/ja809598r ↗
2. 10.1039/c1nr10867k10.1039/c1nr10867k ↗
3. 10.1038/srep0059110.1038/srep00591 ↗
4. 10.1126/science.124316710.1126/science.1243167 ↗
5. 10.1038/ncomms376110.1038/ncomms3761 ↗
6. 10.1126/science.124398210.1126/science.1243982 ↗
7. 10.1038/ncomms770010.1038/ncomms7700 ↗
8. 10.1021/jacs.5b0199410.1021/jacs.5b01994 ↗
9. 10.1039/c3ee40810h10.1039/c3ee40810h ↗
10. 10.1038/nphoton.2013.8010.1038/nphoton.2013.80 ↗
11. 10.1002/adfm.20130209010.1002/adfm.201302090 ↗
12. 10.1038/nphoton.2013.34110.1038/nphoton.2013.341 ↗
13. 10.1021/nn406020d10.1021/nn406020d ↗
14. 10.1039/C4EE01216J10.1039/C4EE01216J ↗
15. 10.1039/C5EE00120J10.1039/C5EE00120J ↗
16. 10.1039/C4EE02441A10.1039/C4EE02441A ↗
17. 10.1063/1.292477110.1063/1.2924771 ↗
18. 10.1002/adma.20100367310.1002/adma.201003673 ↗
19. 10.1021/nl501981f10.1021/nl501981f ↗
20. 10.1039/C5EE00749F10.1039/C5EE00749F ↗
21. 10.1063/1.220988710.1063/1.2209887 ↗
22. 10.1021/jacs.5b0373910.1021/jacs.5b03739 ↗
23. 10.1002/adfm.20120187810.1002/adfm.201201878 ↗
24. 10.1016/j.solmat.2014.08.00910.1016/j.solmat.2014.08.009 ↗
25. 10.1063/1.339467910.1063/1.3394679 ↗
26. 10.1039/C4TA05294C10.1039/C4TA05294C ↗
27. 10.1002/adfm.20100229010.1002/adfm.201002290 ↗
28. 10.1039/c3ee41077c10.1039/c3ee41077c ↗
29. 10.1021/acsami.5b0317110.1021/acsami.5b03171 ↗
30. 10.1002/adma.20150114510.1002/adma.201501145 ↗
31. 10.1002/smll.20140334810.1002/smll.201403348 ↗
32. 10.1038/srep0538010.1038/srep05380 ↗
33. 10.1021/jacs.5b0493010.1021/jacs.5b04930 ↗
34. 10.1039/c3ta13579a10.1039/c3ta13579a ↗
35. 10.1002/adfm.20120099310.1002/adfm.201200993 ↗
36. 10.1103/PhysRevB.82.03531110.1103/PhysRevB.82.035311 ↗
37. 10.1007/s13233-013-1009-610.1007/s13233-013-1009-6 ↗
38. 10.1039/C5EE01179E10.1039/C5EE01179E ↗
39. 10.1126/science.aaa927210.1126/science.aaa9272 ↗
40. 10.1126/science.aaa047210.1126/science.aaa0472 ↗
41. 10.1063/1.490151010.1063/1.4901510 ↗
42. 10.1021/ja411509g10.1021/ja411509g ↗
43. 10.1002/adma.20100409910.1002/adma.201004099 ↗
44. 10.1002/adma.20130132710.1002/adma.201301327 ↗