Relations between Structure, Activity and Stability in C3N4 Based Photocatalysts Used for Solar Hydrogen Production

dc.bibliographicCitation.firstPage52
dc.bibliographicCitation.issue2
dc.bibliographicCitation.journalTitleCatalysts : open access journaleng
dc.bibliographicCitation.volume8
dc.contributor.authorSivasankaran, Ramesh P.
dc.contributor.authorRockstroh, Nils
dc.contributor.authorHollmann, Dirk
dc.contributor.authorKreyenschulte, Carsten R.
dc.contributor.authorAgostini, Giovanni
dc.contributor.authorLund, Henrik
dc.contributor.authorAcharjya, Amitava
dc.contributor.authorRabeah, Jabor
dc.contributor.authorBentrup, Ursula
dc.contributor.authorJunge, Henrik
dc.contributor.authorThomas, Arne
dc.contributor.authorBrückner, Angelika
dc.date.accessioned2023-01-19T09:43:51Z
dc.date.available2023-01-19T09:43:51Z
dc.date.issued2018-1-29
dc.description.abstractSolar hydrogen production from water could be a sustainable and environmentally friendly alternative to fossil energy carriers, yet so far photocatalysts active and stable enough for large-scale applications are not available, calling for advanced research efforts. In this work, H2 evolution rates of up to 1968 and 5188 μmol h−1 g−1 were obtained from aqueous solutions of triethanolamine (TEOA) and oxalic acid (OA), respectively, by irradiating composites of AgIn5S8 (AIS), mesoporous C3N4 (CN, surface area >150 m2/g) and ≤2 wt.% in-situ photodeposited Pt nanoparticles (NPs) with UV-vis (≥300 nm) and pure visible light (≥420 nm). Structural properties and electron transport in these materials were analyzed by XRD, STEM-HAADF, XPS, UV-vis-DRS, ATR-IR, photoluminescence and in situ-EPR spectroscopy. Initial H2 formation rates were highest for Pt/CN, yet with TEOA this catalyst deactivated by inclusion of Pt NPs in the matrix of CN (most pronounced at λ ≥ 300 nm) while it remained active with OA, since in this case Pt NPs were enriched on the outermost surface of CN. In Pt/AIS-CN catalysts, Pt NPs were preferentially deposited on the surface of the AIS phase which prevents them from inclusion in the CN phase but reduces simultaneously the initial H2 evolution rate. This suggests that AIS hinders transport of separated electrons from the CN conduction band to Pt NPs but retains the latter accessible by protons to produce H2.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/10934
dc.identifier.urihttp://dx.doi.org/10.34657/9960
dc.language.isoeng
dc.publisherBasel : MDPI
dc.relation.doihttps://doi.org/10.3390/catal8020052
dc.relation.essn2073-4344
dc.rights.licenseCC BY 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subject.ddc540
dc.subject.otherAgIn5S8eng
dc.subject.otherC3N4eng
dc.subject.otherIn situ-EPReng
dc.subject.otherPhotocatalytic hydrogen productioneng
dc.subject.otherTEMeng
dc.subject.otherXPSeng
dc.titleRelations between Structure, Activity and Stability in C3N4 Based Photocatalysts Used for Solar Hydrogen Productioneng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorLIKAT
wgl.subjectChemieger
wgl.typeZeitschriftenartikelger
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