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Preparation of CIGS thin films by HiPIMS or DC sputtering and various selenization processes

  1. 1.
    SYSNO ASEP0397887
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitlePreparation of CIGS thin films by HiPIMS or DC sputtering and various selenization processes
    Author(s) Olejníček, Jiří (FZU-D) RID, ORCID
    Hubička, Zdeněk (FZU-D) RID, ORCID, SAI
    Kšírová, Petra (FZU-D) RID, ORCID
    Kment, Štěpán (FZU-D) RID, ORCID
    Brunclíková, Michaela (FZU-D) RID
    Kohout, Michal (FZU-D) RID, ORCID
    Čada, Martin (FZU-D) RID, ORCID, SAI
    Darveau, S.A. (US)
    Exstrom, C.L. (US)
    Source TitleJournal of Advanced Oxidation Technologies - ISSN 1203-8407
    Roč. 16, č. 2 (2013), s. 314-319
    Number of pages6 s.
    Languageeng - English
    CountryCA - Canada
    KeywordsCIGS ; HIPIMS ; selenization ; nanocrystals ; solar energy ; sputtering ; thin films
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsLH12045 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Institutional supportFZU-D - RVO:68378271
    UT WOS000322719200014
    EID SCOPUS84881502019
    AnnotationCuIn1-xGaxSe2 (CIGS) thin films were prepared by the sputtering of metallic precursors Cu, In, Ga in HiPIMS or DC magnetron and subsequently selenized in an atmosphere of pure Se or Ar+Se. The average absorbed power and discharge current were the same in the HiPIMS and DC plasma. The basic aim of this work was to compare the structural properties of the CIGS films as a function of magnetron excitation mode and selenization thermal treatment conditions. Film characteristics were measured using X-ray diffraction, scanning electron microscopy, Raman spectroscopy, energy-dispersive X-ray spectroscopy and other techniques. All the CIGS films revealed the chalcopyrite crystal structure with a preferential (112) orientation. Only a very small influence of magnetron excitation mode on thin film properties was observed. On the other hand, selenization in Ar+Se atmosphere led to bigger grain size, better crystallinity and a significantly higher level of Ga substitution.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2014
Number of the records: 1  

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