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Gas Quenching‐Mediated Crystallization for Optoelectronic‐Grade Pb–Sn Perovskite Films

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2026

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Deutsche Forschungsgemeinschaft (DFG): ID0EGFBG33281
Institutionen der Bundesrepublik Deutschland: 03EE1113C
Deutsche Forschungsgemeinschaft (DFG): 533867117

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Solar RRL. Wiley. 2026, 10(6), e202500713. ISSN 2367-198X. eISSN 2367-198X. Verfügbar unter: doi: 10.1002/solr.202500713

Zusammenfassung

The fabrication of narrow‐bandgap (NBG) Pb–Sn perovskites, with bandgaps typically around 1.1–1.3 eV, is often challenging due to issues related to repeatability, stability, and rapid crystallization kinetics. While Sn–Pb perovskites offer advantages such as defect tolerance and lower toxicity, they are also prone to inhomogeneous crystallization. Sn‐based component of perovskite crystallizes much faster than the Pb‐based component, leading to poor film coverage, pinholes, and rough morphologies. In this study, we employed gas quenching (GQ) instead of the commonly used antisolvent (AS) quenching to address the rapid crystallization issue. GQ approach resulted in slower crystallization and improved film quality. Besides, GQ produced more reproducible results compared to AS quenching. Devices fabricated using the GQ method also demonstrated better performance with higher open‐circuit voltage (VOC) values. Specifically, devices prepared with the AS method achieved a power conversion efficiency (PCE) of 18.3%, whereas those using the GQ method reached a PCE of 19.1%. This improvement in efficiency combined with enhanced reproducibility, the simplicity, and environmental friendliness of the GQ approach underscores its advantage for processing NBG Pb–Sn mixed perovskite films. Therefore, the GQ method holds significant potential for application in the fabrication of NBG Pb–Sn perovskite solar cells.

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530 Physik

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ISO 690TEMITMIE, Yekitwork Abebe, Maria AZHAR, Muhammad Irfan HAIDER, Yenal YALCINKAYA, Emilia R. SCHÜTZ, Tim MAYER, Amare BENOR, Lukas SCHMIDT-MENDE, 2026. Gas Quenching‐Mediated Crystallization for Optoelectronic‐Grade Pb–Sn Perovskite Films. In: Solar RRL. Wiley. 2026, 10(6), e202500713. ISSN 2367-198X. eISSN 2367-198X. Verfügbar unter: doi: 10.1002/solr.202500713
BibTex
@article{Temitmie2026-03-29Quenc-76220,
  title={Gas Quenching‐Mediated Crystallization for Optoelectronic‐Grade Pb–Sn Perovskite Films},
  year={2026},
  doi={10.1002/solr.202500713},
  number={6},
  volume={10},
  issn={2367-198X},
  journal={Solar RRL},
  author={Temitmie, Yekitwork Abebe and Azhar, Maria and Haider, Muhammad Irfan and Yalcinkaya, Yenal and Schütz, Emilia R. and Mayer, Tim and Benor, Amare and Schmidt-Mende, Lukas},
  note={Article Number: e202500713}
}
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    <dcterms:abstract>The fabrication of narrow‐bandgap (NBG) Pb–Sn perovskites, with bandgaps typically around 1.1–1.3 eV, is often challenging due to issues related to repeatability, stability, and rapid crystallization kinetics. While Sn–Pb perovskites offer advantages such as defect tolerance and lower toxicity, they are also prone to inhomogeneous crystallization. Sn‐based component of perovskite crystallizes much faster than the Pb‐based component, leading to poor film coverage, pinholes, and rough morphologies. In this study, we employed gas quenching (GQ) instead of the commonly used antisolvent (AS) quenching to address the rapid crystallization issue. GQ approach resulted in slower crystallization and improved film quality. Besides, GQ produced more reproducible results compared to AS quenching. Devices fabricated using the GQ method also demonstrated better performance with higher open‐circuit voltage (V&lt;sub&gt;OC&lt;/sub&gt;) values. Specifically, devices prepared with the AS method achieved a power conversion efficiency (PCE) of 18.3%, whereas those using the GQ method reached a PCE of 19.1%. This improvement in efficiency combined with enhanced reproducibility, the simplicity, and environmental friendliness of the GQ approach underscores its advantage for processing NBG Pb–Sn mixed perovskite films. Therefore, the GQ method holds significant potential for application in the fabrication of NBG Pb–Sn perovskite solar cells.</dcterms:abstract>
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