Carbazole-Based Spiro[fluorene-9,9′-xanthene] as an Efficient Hole-Transporting Material for Perovskite Solar Cells
Source abstract
Abstract
For the practical application of perovskite solar cells (PSC), it is desirable to have high efficiency, long-term stability, and low manufacturing cost. Therefore, it is required to develop inexpensive and well-performing hole-transporting materials (HTMs). In this study, we synthesized SFXDAnCBZ, which is a new carbazole-based spiro[fluorene-9,9′-xanthene] (SFX) derivative, where the central core and end-cap units consist of SFX and N3,N6-bis(di-4-anisylamino)-9H-carbazole (DAnCBZ), respectively, as an efficient and low-cost HTM for PSCs. Photoluminescence quenching at the SFXDAnCBZ/perovskite interface was more effective than at the perovskite/Spiro-OMeTAD (2,2′,7,7′-tetrakis-(N,N-di-p-methoxy-phenyl-amine) 9,9′spiro-bifluorene) interface. We fabricated a PSC with a power conversion efficiency (PCE) of 20.87% under 1 sun illumination (100 mW cm–2) using SFXDAnCBZ as an HTM. This value is comparable to that measured for the benchmark Spiro-OMeTAD. Thus, this result confirms that SFX core-based materials can be a new kind of HTMs for high-efficiency and low-cost PSCs.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Organic Light-Emitting Diodes Research · Conducting polymers and applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Chemistry and Energy Engineering, School of Energy and Chemical Engineering, Ulsan National Institute of Science and Technology (UNIST), Ulsan 44919, Republic of Korea
Department of Chemistry, Indian Institute of Technology, Indore 453552, India
Funding
Science and Engineering Research Board · National Research Foundation of Korea · Department of Science and Technology, Ministry of Science and Technology
References (24)
Show source-provided references
1. 10.1038/nature1413310.1038/nature14133 ↗
2. 10.1126/science.122860410.1126/science.1228604 ↗
3. 10.1038/nphoton.2013.8010.1038/nphoton.2013.80 ↗
4. 10.1002/aenm.20150021310.1002/aenm.201500213 ↗
5. 10.1021/jacs.6b0629110.1021/jacs.6b06291 ↗
6. 10.1126/science.aay704410.1126/science.aay7044 ↗
7. 10.1002/aenm.20170026410.1002/aenm.201700264 ↗
8. 10.1039/C6TA09028A10.1039/C6TA09028A ↗
9. 10.1038/nenergy.2015.1710.1038/nenergy.2015.17 ↗
10. 10.1021/ol060871z10.1021/ol060871z ↗
11. 10.1039/C6TA00110F10.1039/C6TA00110F ↗
12. 10.1039/C8TA08503J10.1039/C8TA08503J ↗
13. 10.1016/j.nanoen.2016.03.02010.1016/j.nanoen.2016.03.020 ↗
14. 10.1016/j.chempr.2017.03.01110.1016/j.chempr.2017.03.011 ↗
15. 10.1021/am404948w10.1021/am404948w ↗
16. 10.1021/jo301653810.1021/jo3016538 ↗
17. 10.1002/adfm.20170435110.1002/adfm.201704351 ↗
18. 10.1039/C7CC08985F10.1039/C7CC08985F ↗
19. 10.1002/advs.20170081110.1002/advs.201700811 ↗
20. 10.1021/acs.jpcc.8b0948210.1021/acs.jpcc.8b09482 ↗
21. 10.1002/cssc.20170097310.1002/cssc.201700973 ↗
22. 10.1039/C7CC04606E10.1039/C7CC04606E ↗
23. 10.1039/C7TA04762B10.1039/C7TA04762B ↗
24. 10.1039/C6TA00976J10.1039/C6TA00976J ↗