Scope for Spherical Bi2WO6 Quazi-Perovskites in the Artificial Photosynthesis Reaction—The Effects of Surface Modification with Amine Groups

The synthesis, characterisation, modification (with n-propyl amine groups) of Bi 2 WO 6 particles and the scope for their application in artificial photosynthesis reactions is described. The synthesis involves microwave activation of spherical Bi 2 O 3 precursors followed by a hydrothermal treatment...

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Veröffentlicht in:Catalysis letters 2021, Vol.151 (1), p.293-305
Hauptverfasser: Morais, Eduardo, Stanley, Kristy, Thampi, K. Ravindranathan, Sullivan, James A.
Format: Artikel
Sprache:eng
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Zusammenfassung:The synthesis, characterisation, modification (with n-propyl amine groups) of Bi 2 WO 6 particles and the scope for their application in artificial photosynthesis reactions is described. The synthesis involves microwave activation of spherical Bi 2 O 3 precursors followed by a hydrothermal treatment in the presence of Na 2 WO 4 . These are characterised using electron microscopy (TEM and SEM), BET, XRD, FTIR, FT-Raman and UV–Visible spectroscopies and CO 2 TPD. Subsequently this material is modified through the condensation of propyl amine groups to surface hydroxyl groups, and the composites prepared are characterised using FTIR and D-FTIR following exposure to CO 2 . Both the spherical particles and the amine-modified analogues are applied in the artificial photosynthesis reaction under batch conditions. O 2 , CO and CH 4 are the observed gaseous products during the reaction and there is FTIR evidence for the formation of adsorbed alcohols and carbonylated products. Although the modification with amine groups decreased the overall photocatalytic reactivity, it also altered the product selectivity with respect to the CH 4 /CO ratio. The catalyst tends to improve the oxygen production ability after about 20 h of operation, with a decline in CH 4 and CO production, indicating that other condensates are probably generated. This opens up new possibilities and scope for this catalyst and further research is required to understand the observations. Graphic Abstract
ISSN:1011-372X
1572-879X
DOI:10.1007/s10562-020-03299-5