Inverted J – V Hysteresis in Perovskite Solar Cells: Insights from Photovoltaic Quantum Efficiency
Source abstract
Abstract
The most typical hysteresis in the current density-voltage (J-V) curve of perovskite solar cells (PSCs) shows better performance in the backward (BW) than in the forward (FW) voltage scan (normal hysteresis). The opposite, where the FW scan yields higher photocurrent, is known as inverted hysteresis and is also frequently observed. Here, we examine PSCs exhibiting both normal and inverted hysteresis, depending on scan rate and preconditioning. Spectral changes in the external quantum efficiency (EQE) linked to ionic redistribution reveal that inverted hysteresis arises from blue-range photocurrent losses caused by enhanced recombination at the interfaces due to ionic accumulation. This trend is consistent across PSC architectures, as demonstrated for triple mesoscopic carbon-based (C-PSCs) and planar p-i-n devices. Combined with drift-diffusion simulations, the results show that ionic losses can be bidirectional, and the hysteresis direction depends on how the ionic distribution impacts charge collection efficiency.
Source: europepmc · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: Perovskite Materials and Applications · TiO2 Photocatalysis and Solar Cells · Organic Electronics and Photovoltaics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institute of Computational Physics
Zurich University of Applied Sciences (ZHAW)
Institut des Matériaux, École Polytechnique Fédérale de Lausanne (EPFL)
Swansea University, Bay Campus, Neath, Skewen SA18EN, Wales
Funding
H2020 European Research Council
References (25)
Show source-provided references
1. 10.1039/C4EE03664F10.1039/C4EE03664F ↗
2. 10.1002/ange.20170172410.1002/ange.201701724 ↗
3. 10.1039/C8EE01576G10.1039/C8EE01576G ↗
4. 10.1039/D5EL00133A10.1039/D5EL00133A ↗
5. 10.1002/solr.20210077210.1002/solr.202100772 ↗
6. 10.1039/D5EL00137D10.1039/D5EL00137D ↗
7. 10.1039/D4EE02669A10.1039/D4EE02669A ↗
8. 10.1021/acsenergylett.5c0243510.1021/acsenergylett.5c02435 ↗
9. 10.1002/aenm.20160039610.1002/aenm.201600396 ↗
10. 10.1021/acs.jpcc.7b0424810.1021/acs.jpcc.7b04248 ↗
11. 10.1021/acsenergylett.8b0160610.1021/acsenergylett.8b01606 ↗
12. 10.1063/5.013668310.1063/5.0136683 ↗
13. 10.1126/science.adj708110.1126/science.adj7081 ↗
14. 10.1038/s41560-024-01689-210.1038/s41560-024-01689-2 ↗
15. 10.1038/ncomms1383110.1038/ncomms13831 ↗
16. 10.1038/s41560-024-01487-w10.1038/s41560-024-01487-w ↗
17. 10.1021/acs.jpclett.7b0057110.1021/acs.jpclett.7b00571 ↗
18. 10.1039/C6CP06989D10.1039/C6CP06989D ↗
19. 10.1016/j.solmat.2019.03.00310.1016/j.solmat.2019.03.003 ↗
20. 10.1021/acs.jpclett.0c0233110.1021/acs.jpclett.0c02331 ↗
21. 10.1002/aenm.20240385010.1002/aenm.202403850 ↗
22. 10.1016/j.joule.2019.10.00310.1016/j.joule.2019.10.003 ↗
23. 10.1021/acs.jpclett.5c0140510.1021/acs.jpclett.5c01405 ↗
24. 10.1039/C7EE02048A10.1039/C7EE02048A ↗
25. 10.1021/acsenergylett.4c0014010.1021/acsenergylett.4c00140 ↗