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Electron transport bilayer with cascade energy alignment based on Nb 2 O 5 –Ti 3 C 2 MXene/TiO 2 for efficient perovskite solar cells
Nb 2 O 5 shows promising features for electron transport layers (ETL) in perovskite solar cells (PSCs), such as suitable band alignment and ultraviolet stability. Here, we studied the incorporation of Ti 3 C 2 T x MXene in a solution-processable compact layer as a component of ETLs for PSCs. The add...
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Published in: | Journal of materials chemistry. C, Materials for optical and electronic devices Materials for optical and electronic devices, 2023-03, Vol.11 (10), p.3571-3580 |
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Main Authors: | , , , , , , , , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Nb
2
O
5
shows promising features for electron transport layers (ETL) in perovskite solar cells (PSCs), such as suitable band alignment and ultraviolet stability. Here, we studied the incorporation of Ti
3
C
2
T
x
MXene in a solution-processable compact layer as a component of ETLs for PSCs. The addition of 0.4 wt% MXene with respect to niobium ethoxide was shown to enhance the PCE (19.46% for the champion device) and stability (96% of its original PCE after 500 hours) compared to pristine devices. The improved performance of the Nb
2
O
5
–Ti
3
C
2
devices (0.4 wt%) could be attributed to the adapted alignment of the energy band between perovskite and ETL layers, which favors electron transport and extraction. In addition, the high electrical conductivity of MXenes worked as a free pathway for the extracted electrons preventing charge recombination. These features were corroborated by Photo-CELIV, which showed a higher density of extracted charges and increased charge carrier lifetime for Nb
2
O
5
–Ti
3
C
2
based devices. Hence, the results unveiled in this work indicate that MXenes are promising 2D materials for tuning Nb
2
O
5
based ETLs. Future works shall focus on other MXene compounds to further boost PSC performance and stability. |
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ISSN: | 2050-7526 2050-7534 |
DOI: | 10.1039/D3TC00022B |