Reliable Measurement of Ionic and Electronic Defects in Inorganic CsPbBr 3 Perovskite Solar Cells
Source abstract
Abstract
High Resolution Image Download MS PowerPoint Slide Metal halide perovskites demonstrate exceptional optoelectronic properties but face stability issues due to ion migration. This study investigates ion density, ion mobility, and electronic defects in CsPbBr 3 devices with and without organic p-layers, by using Bias-Assisted Charge Extraction (BACE) and Mott–Schottky methods over temperatures of 25 to 125 °C. We find that reliable estimates of mobile ion density through Mott–Schottky and BACE methods are only achieved under conditions that fully activate the ionic response. Elevated temperatures induce thermal activation of ionic responses by increasing mobility, allowing consistent quantification of ion parameters. BACE measurements demonstrate that ion mobility and concentration increase with temperature, and Br – activation energies can be calculated through ion time-of-flight. Alternatively, Mott–Schottky measurements exhibit high- and low-frequency plateaus corresponding to electronic and ionic defects, respectively. We show that organic hole transport layers induce measurement inaccuracies and larger mobile ion concentrations, whereas devices without these layers do not exhibit the same issues.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Thermal Expansion and Ionic Conductivity · Optical properties and cooling technologies in crystalline materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Electrical and Computer Engineering
Iowa State University
Funding
Iowa State University · Micron Research Foundation
References (38)
Show source-provided references
1. 10.1038/s41377-022-01010-410.1038/s41377-022-01010-4 ↗
2. 10.1002/pip.391910.1002/pip.3919 ↗
3. 10.1039/C6EE00413J10.1039/C6EE00413J ↗
4. 10.1038/s41467-019-09079-z10.1038/s41467-019-09079-z ↗
5. 10.1088/2053-1591/ab4d7910.1088/2053-1591/ab4d79 ↗
6. 10.1002/aenm.20160292210.1002/aenm.201602922 ↗
7. 10.1021/acsnano.5b0368710.1021/acsnano.5b03687 ↗
8. 10.1038/s41560-024-01487-w10.1038/s41560-024-01487-w ↗
9. 10.1021/acs.jpclett.2c0080410.1021/acs.jpclett.2c00804 ↗
10. 10.1063/1.513275410.1063/1.5132754 ↗
11. 10.1063/1.506325910.1063/1.5063259 ↗
12. 10.1021/acs.jpclett.3c0053010.1021/acs.jpclett.3c00530 ↗
13. 10.1021/acsenergylett.4c0244610.1021/acsenergylett.4c02446 ↗
14. 10.1021/acsaem.2c0062410.1021/acsaem.2c00624 ↗
15. 10.1021/acsaem.0c0001010.1021/acsaem.0c00010 ↗
16. 10.1039/D4TC00973H10.1039/D4TC00973H ↗
17. 10.1016/j.solmat.2023.11238710.1016/j.solmat.2023.112387 ↗
18. 10.1063/1.512903710.1063/1.5129037 ↗
19. 10.1021/acs.jpcc.7b0671110.1021/acs.jpcc.7b06711 ↗
20. 10.1039/D4EE02494J10.1039/D4EE02494J ↗
21. 10.1021/acsenergylett.5c0088710.1021/acsenergylett.5c00887 ↗
22. 10.1021/acs.jpcc.8b0325510.1021/acs.jpcc.8b03255 ↗
23. 10.1021/acs.jpcc.5b1162710.1021/acs.jpcc.5b11627 ↗
24. 10.1002/smtd.20250055410.1002/smtd.202500554 ↗
25. 10.1021/acsami.6b0775010.1021/acsami.6b07750 ↗
26. 10.1557/opl.2012.51210.1557/opl.2012.512 ↗
27. 10.1016/j.joule.2020.01.01210.1016/j.joule.2020.01.012 ↗
28. 10.1038/ncomms849710.1038/ncomms8497 ↗
29. 10.1063/5.018001310.1063/5.0180013 ↗
30. 10.1063/5.024979010.1063/5.0249790 ↗
31. 10.1002/solr.20210077210.1002/solr.202100772 ↗
32. 10.1126/science.aba089310.1126/science.aba0893 ↗
33. 10.1126/science.abd801410.1126/science.abd8014 ↗
34. 10.1126/science.abd859810.1126/science.abd8598 ↗
35. 10.1021/acsenergylett.1c0144910.1021/acsenergylett.1c01449 ↗
36. 10.1063/5.012354710.1063/5.0123547 ↗
37. 10.1103/PRXEnergy.2.04301110.1103/PRXEnergy.2.043011 ↗
38. 10.1021/acsaem.4c0219410.1021/acsaem.4c02194 ↗