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Cited 5 time in webofscience Cited 6 time in scopus
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In Search of Disorder Transitions and Defects Within Cu2ZnSn(S,Se)4-Based Absorber Layers via Temperature-Dependent Raman Spectroscopy Technique

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dc.contributor.authorGour, K.S.-
dc.contributor.authorKarade, V.C.-
dc.contributor.authorParmar, R.-
dc.contributor.authorJang, J.S.-
dc.contributor.authorKazim, S.-
dc.contributor.authorJang, S.-
dc.contributor.authorGunnella, R.-
dc.contributor.authorPark, J.-
dc.contributor.authorYun, J.H.-
dc.contributor.authorKim, J.H.-
dc.date.accessioned2023-05-03T06:40:48Z-
dc.date.available2023-05-03T06:40:48Z-
dc.date.issued2023-06-
dc.identifier.issn2367-198X-
dc.identifier.issn2367-198X-
dc.identifier.urihttps://scholarworks.gnu.ac.kr/handle/sw.gnu/59346-
dc.description.abstractThe temperature-dependent (25–300 °C) disorder transitions analyzed via Raman spectroscopic technique for the different non-stoichiometric Cu2ZnSn(S,Se)4 (CZTSSe) thin films are demonstrated. In the thin films prepared with different Zn conditions, i.e., in Zn-1 (Zn-poor), the density of the A-type defect cluster [ZnCu + VCu] increases with temperature; however, it slightly decreases and remains constant for Zn-rich samples, i.e., Zn-2 and Zn-3. At the same time, the density of the B-type defect cluster [2ZnCu + ZnSn] increases with increasing temperature and Zn content. The observations further reveal that Zn concentration has less impact on VCu formation; therefore, above the optimum Cu-poor and Zn-rich conditions, ZnCu shallow donors negatively influence the kesterite device performances. Finally, solar cells based on all the CZTSSe thin-film samples (Zn-1, Zn-2, and Zn-3) are fabricated in which a device based on Zn-2 exhibits excellent power conversion efficiency of ≈11.0% with open-circuit voltage of 478 mV, short-circuit current of 35.51 mA cm−2, and fill factor of 64%, respectively. © 2023 Wiley-VCH GmbH.-
dc.language영어-
dc.language.isoENG-
dc.publisherJohn Wiley and Sons Inc-
dc.titleIn Search of Disorder Transitions and Defects Within Cu2ZnSn(S,Se)4-Based Absorber Layers via Temperature-Dependent Raman Spectroscopy Technique-
dc.typeArticle-
dc.publisher.location독일-
dc.identifier.doi10.1002/solr.202200946-
dc.identifier.scopusid2-s2.0-85153224890-
dc.identifier.wosid000974035100001-
dc.identifier.bibliographicCitationSolar RRL, v.7, no.12-
dc.citation.titleSolar RRL-
dc.citation.volume7-
dc.citation.number12-
dc.type.docTypeArticle-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaEnergy & Fuels-
dc.relation.journalResearchAreaMaterials Science-
dc.relation.journalWebOfScienceCategoryEnergy & Fuels-
dc.relation.journalWebOfScienceCategoryMaterials Science, Multidisciplinary-
dc.subject.keywordPlusKESTERITE SOLAR-CELLS-
dc.subject.keywordPlusTHIN-FILMS-
dc.subject.keywordPlusFUTURE-PROSPECTS-
dc.subject.keywordPlusCU2ZNSNS4-
dc.subject.keywordPlusEFFICIENCY-
dc.subject.keywordPlusCZTSSE-
dc.subject.keywordPlusSCATTERING-
dc.subject.keywordPlusPRECURSOR-
dc.subject.keywordPlusNA-
dc.subject.keywordAuthordefects-
dc.subject.keywordAuthorefficiency-
dc.subject.keywordAuthorkesterites-
dc.subject.keywordAuthortemperature-dependent Raman spectroscopy-
dc.subject.keywordAuthorXPS-
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