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Generating a Stable Higher-Symmetry CsPbI₃ Perovskite Phase in Ambient Conditions: Unveiling the Stabilization Mechanism

 
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cris.virtual.orcid0000-0002-4019-5979
cris.virtual.orcid0000-0002-9299-9784
cris.virtual.orcid0000-0003-0079-7884
cris.virtual.orcid0000-0003-0403-602X
cris.virtualsource.department73187a2f-4799-45d3-9ae1-7cd599fe36b8
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cris.virtualsource.departmentbb3b1585-80d2-4987-bed1-dd87e7bde84b
cris.virtualsource.orcid73187a2f-4799-45d3-9ae1-7cd599fe36b8
cris.virtualsource.orcidbbd0a143-3b19-4b7f-9376-6819b58ed5d9
cris.virtualsource.orcideae674d6-b3a6-4326-8856-0595ff358cb1
cris.virtualsource.orcidbb3b1585-80d2-4987-bed1-dd87e7bde84b
dc.contributor.authorAli Saha Rafikul
dc.contributor.authorPapadopoulou, Athina
dc.contributor.authorAriza, Rocio
dc.contributor.authorDegutis, Giedrius
dc.contributor.authorSkvortsova, Irina
dc.contributor.authorBraeckevelt, Tom
dc.contributor.authorDe Angelis Francesco
dc.contributor.authorSolano Minuesa Eduardo
dc.contributor.authorGouveia dos Anjos, Joao Pedro de Sousa
dc.contributor.authorPintor Monroy, Isabel
dc.contributor.authorMongilyov, Ilya
dc.contributor.authorGoderis, Bart
dc.contributor.authorRubio-Zuazo, Juan
dc.contributor.authorGenoe, Jan
dc.contributor.authorMeneghini, Carlo
dc.contributor.authorSteele, Julian A.
dc.contributor.authorBals, Sara
dc.contributor.authorVan Speybroeck Veronique
dc.contributor.authorHofkens, Johan
dc.contributor.authorRoeffaers, Maarten
dc.contributor.imecauthorPapadopoulou, Athina
dc.contributor.imecauthorDegutis, Giedrius
dc.contributor.imecauthorPintor Monroy, Maria Isabel
dc.contributor.imecauthorGenoe, Jan
dc.contributor.orcidimecPapadopoulou, Athina::0000-0003-0079-7884
dc.contributor.orcidimecDegutis, Giedrius::0000-0002-9299-9784
dc.contributor.orcidimecGenoe, Jan::0000-0002-4019-5979
dc.date.accessioned2025-08-10T03:59:09Z
dc.date.available2025-08-10T03:59:09Z
dc.date.issued2025
dc.description.abstractBlack-phase cesium lead iodide (CsPbI3) is a promising candidate for high-efficiency perovskite optoelectronics, but its instability under ambient conditions remains a major challenge. Among several strategies, dimethylammonium iodide (DMAI) has emerged as a potential stabilizer; however, inconsistencies in phase stability (3-7 days) and lower solar power conversion efficiencies (similar to 20 vs similar to 27% for hybrid perovskites) highlight the need for further improvements. This study not only demonstrates enhanced stabilization of the high-symmetry black phase of CsPbI3 and improved film morphology through optimized composition and annealing conditions but also more importantly provides detailed mechanistic insights obtained from comprehensive experimental and theoretical analyses. Systematic tuning of the DMAI concentration (1.2 M), annealing temperature (200 degrees C, 1 min), and Cs+ substitution (12-15%) significantly extends phase stability to 7 days under ambient conditions (35-52% relative humidity) and maintains stability even after 16 months in a drybox environment by reducing orthorhombic strain and octahedral tilting. Additionally, a minor (similar to 5%) zero-dimensional (0D) Cs4PbI6 phase fills pinholes, enhancing the film quality. Optimized photodiodes exhibit a low dark current (similar to 1 mu A/cm2), high external quantum efficiency (similar to 80% at -2 V), and a >= 100 dB linear dynamic range. These findings provide mechanistic insights into the stabilization of the black phase of CsPbI3, advancing the development of more stable and efficient perovskite-based optoelectronic devices.
dc.description.wosFundingTextThis work was supported by iBOF-21-085 PERsist and Internal Funds KU Leuven (C14/23/090). The authors acknowledge financial support from the Fund for Scientific Research Flanders (FWO) under Project Numbers S004322N (GigaPixel) and G0A5923N (SUSTRAINABLE). I.S. acknowledges the SB-FWO Project 1SHA024N for funding. V.V.S. acknowledges the Research Fund of Ghent University (BOF) for its financial support. The computational resources and services used in this work were provided by VSC (Flemish Supercomputer Center), funded by the Research Foundation-Flanders (FWO), and the Flemish Government. R.A.S., E.S., and J.A.S. thank the staff of the BL11 NCD-SWEET beamline for their assistance in recording the synchrotron GIWAXS data. R.A.S., C.M., and F.D.A. acknowledge Dr. Cesare Atzori for his help during the XAFS measurement. The authors acknowledge the ESRF for beamtime at BM23 and BM25. R.A. acknowledges financial support from Marie Sklodowska-Curie Grant Agreement No. 101149132.
dc.identifier.doi10.1021/acsnano.5c07700
dc.identifier.issn1936-0851
dc.identifier.pmidMEDLINE:40728153
dc.identifier.urihttps://imec-publications.be/handle/20.500.12860/46050
dc.publisherAMER CHEMICAL SOC
dc.source.beginpage28540
dc.source.endpage28553
dc.source.issue19
dc.source.journalACS NANO
dc.source.numberofpages14
dc.source.volume31
dc.subject.keywordsSPONTANEOUS STRAIN
dc.subject.keywordsSOLAR-CELLS
dc.subject.keywordsCESIUM
dc.title

Generating a Stable Higher-Symmetry CsPbI₃ Perovskite Phase in Ambient Conditions: Unveiling the Stabilization Mechanism

dc.typeJournal article
dspace.entity.typePublication
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