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Dopant site in indium-doped SrTiO3 photocatalysts

  • Hanggara Sudrajat (Corresponding author)
  • , Mohamed M. Fadlallah
  • , Shuxia Tao
  • , Mitsunori Kitta
  • , Nobuyuki Ichikuni
  • , Hiroshi Onishi

    Onderzoeksoutput: Bijdrage aan tijdschriftTijdschriftartikelAcademicpeer review

    Samenvatting

    Strontium titanate, SrTiO3, with the perovskite ABO3 structure is known as one of the most efficient photocatalyst materials for the overall water splitting reaction. Doping with appropriate metal cations at the A site or at the B site substantially increases the quantum yield to split water into H2 and O2. The site occupied by the guest dopant in the SrTiO3 host thus plays a key role in dictating the water splitting activity. However, little is known about the detailed structure of the dopant site in the host lattice. In this study, the local structure of In3+ cations, which were shown to improve the water splitting activity of SrTiO3, is investigated with X-ray absorption fine structure spectroscopy and density functional theory (DFT) calculations. The In3+ cations exclusively substitute for Ti4+ cations at the B site to form InO6 octahedra. Further optical experiments using UV-Vis diffuse reflectance spectroscopy and DFT calculations of the density of states indicate that the substitution of In3+ for Ti4+ does not alter the band structure and bandgap energy (remaining at 3.2 eV). The mechanism underlying the increased water splitting activity is discussed in relation to occupation of the B site by In3+ cations.

    Originele taal-2Engels
    Pagina's (van-tot)19178-19187
    Aantal pagina's10
    TijdschriftPhysical Chemistry Chemical Physics
    Volume22
    Nummer van het tijdschrift34
    DOI's
    StatusGepubliceerd - 14 sep. 2020

    Financiering

    H. S. is an International Research Fellow of the Japan Society for the Promotion of Science (JSPS). The authors acknowledge funding from JSPS KAKENHI (Grants JP18F18029, JP16H02250, JP18KK0161, and JP19H00915). The X-ray absorption measurements were performed under the approval of the Photon Factory Advisory Committee (Proposals 2016G057 and 2018G078). M. M. F. would like to thank Science and Technology Development Fund (STDF), Egypt, (http://www.stdf.org.eg/index.php/en/) for financial support of this scientific research work through the Short-Term Fellowship (STF-25444) project. S. T. acknowledges funding from the Computational Sciences for Energy Research (CSER) tenure track program of Shell and NWO (Project Number 15CST04-2), the Netherlands.

    FinanciersFinanciernummer
    Shell
    Japan Society for the Promotion of ScienceJP19H00915, 2016G057, JP18F18029, 2018G078, JP16H02250, JP18KK0161
    Nederlandse Organisatie voor Wetenschappelijk Onderzoek15CST04-2

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