journal article·2025-05-29

Intrinsic Defect Tolerance in Inorganic Tin–Lead Perovskites

Jiajia Zhang, Xinhao Duan, Zhuang Hu, Xiang Li, Lin Zhang, Shuisheng Chen

Publisher page

Abstract

Experimentally, inorganic tin–lead (Sn–Pb) perovskites exhibit an extremely short carrier lifetime of mere nanoseconds, primarily attributed to strong nonradiative recombination induced by high-density defects. This has led to the belief that they are highly defect-sensitive. Here, we argue that inorganic Sn–Pb perovskites are intrinsically defect-tolerant. We substantiate this claim by performing rigorous first-principles calculations for a prototypical composition CsSn 0.5 Pb 0.5 I 3 . Our results show that this material possesses an ultralong nonradiative lifetime of 10 μs, even under the assumption of a high defect concentration of 10 16 cm –3 . The alteration in band edge energies arising from the mixing of CsSnI 3 and CsPbI 3 is proven to contribute to the remarkable defect tolerance. We ascribe the poor photoelectric performance observed in inorganic Sn–Pb perovskites to inadequate miscibility of their components. This study reveals the inherent superior properties of inorganic Sn–Pb perovskites that have thus far remained unrecognized by the research community and suggests that achieving phase-pure mixing systems is crucial to fully exploit their untapped potential.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · ZnO doping and properties · Gas Sensing Nanomaterials and Sensors

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Anhui Provincial Key Laboratory of Green Carbon Chemistry, School of Chemistry and Materials Engineering

Fuyang Normal University

Funding

Anhui Provincial Department of Education · Fuyang Normal University · National Natural Science Foundation of China · Natural Science Foundation of Anhui Province

References (32)

Show source-provided references
1. 10.1016/j.pmatsci.2023.10122310.1016/j.pmatsci.2023.101223 ↗
2. 10.1126/science.abn567910.1126/science.abn5679 ↗
3. 10.1039/C8EE03559H10.1039/C8EE03559H ↗
4. 10.1016/j.solener.2016.02.01510.1016/j.solener.2016.02.015 ↗
5. 10.1016/j.solener.2023.11182510.1016/j.solener.2023.111825 ↗
6. 10.1038/s41467-019-13908-610.1038/s41467-019-13908-6 ↗
7. 10.1016/j.jechem.2022.05.03010.1016/j.jechem.2022.05.030 ↗
8. 10.1002/adma.20230919310.1002/adma.202309193 ↗
9. 10.1016/j.cej.2023.14755410.1016/j.cej.2023.147554 ↗
10. 10.1021/acsenergylett.2c0243510.1021/acsenergylett.2c02435 ↗
11. 10.1021/acsenergylett.3c0168210.1021/acsenergylett.3c01682 ↗
12. 10.1039/D2EE00288D10.1039/D2EE00288D ↗
13. 10.1021/acs.nanolett.4c0570110.1021/acs.nanolett.4c05701 ↗
14. 10.1021/acs.jpclett.4c0065710.1021/acs.jpclett.4c00657 ↗
15. 10.1021/acs.jpclett.2c0307210.1021/acs.jpclett.2c03072 ↗
16. 10.1002/anie.20221200210.1002/anie.202212002 ↗
17. 10.1021/acs.jpcc.1c0874110.1021/acs.jpcc.1c08741 ↗
18. 10.1103/PhysRevLett.128.13640110.1103/PhysRevLett.128.136401 ↗
19. 10.1038/s41560-021-00949-910.1038/s41560-021-00949-9 ↗
20. 10.1002/anie.20250339410.1002/anie.202503394 ↗
21. 10.1039/D1TA09027E10.1039/D1TA09027E ↗
22. 10.1021/acs.jpclett.9b0278610.1021/acs.jpclett.9b02786 ↗
23. 10.1103/PhysRevB.93.20130410.1103/PhysRevB.93.201304 ↗
24. 10.1021/acsenergylett.8b0067210.1021/acsenergylett.8b00672 ↗
25. 10.1021/ja301539s10.1021/ja301539s ↗
26. 10.1063/5.007060410.1063/5.0070604 ↗
27. 10.1038/s41563-021-00986-510.1038/s41563-021-00986-5 ↗
28. 10.1021/acs.jpclett.0c0072510.1021/acs.jpclett.0c00725 ↗
29. 10.1103/PhysRevB.90.07520210.1103/PhysRevB.90.075202 ↗
30. 10.1021/jacs.0c1306910.1021/jacs.0c13069 ↗
31. 10.1002/anie.20240175110.1002/anie.202401751 ↗
32. 10.1103/PhysRevB.41.824010.1103/PhysRevB.41.8240 ↗