Abstract
Highly dispersed molybdenum oxide supported on mesoporous silica SBA-15 has been prepared by anion exchange resulting in a series of catalysts with changing Mo densities (0.2–2.5 Mo atoms nm−2). X-ray absorption, UV/Vis, Raman, and IR spectroscopy indicate that doubly anchored tetrahedral dioxo MoO4 units are the major surface species at all loadings. Higher reducibility at loadings close to the monolayer measured by temperature-programmed reduction and a steep increase in the catalytic activity observed in metathesis of propene and oxidative dehydrogenation of propane at 8 % of Mo loading are attributed to frustration of Mo oxide surface species and lateral interactions. Based on DFT calculations, NEXAFS spectra at the O-K-edge at high Mo loadings are explained by distorted MoO4 complexes. Limited availability of anchor silanol groups at high loadings forces the MoO4 groups to form more strained configurations. The occurrence of strain is linked to the increase in reactivity.
Only uncomfortable seats left: At high surface coverages of molybdenum oxide, at which surface hydroxy anchoring sites are limited, surface metal oxide molecules are forced to be anchored in strained/frustrated configurations. This strain leads to increased reactivity and explains the non-linear coverage dependence sometimes observed in monolayer-type supported metal oxide catalysts.
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Ligand Redox Noninnocence in [Co III (TAML)] 0/– Complexes Affects Nitrene Formation Nicolaas P. van Leest, Martijn A. Tepaske, Jean-Pierre H. Oudsen, Bas Venderbosch, Niels R. Rietdijk, Maxime A. Siegler, Moniek Tromp, Jarl Ivar van der Vlugt, and Bas de Bruin DOI: 10.1021/jacs.9b11715 J . Am. Chem. Soc. ASAP 訂正 雑誌会スライド8、9枚目の [Co III (TAML sq )] – の有効磁気モーメントの数値が [Co III (TAML red )] – のものになっていましたので、訂正致します。 誤: µ eff = 2.94 µ B ( S =1/2) 正: µ eff = 1.88 µ B ( S =1/2) Evans 法 NMR によって常磁性化合物の磁化率を求める方法。以下の式1– 5によって磁化率、有効磁気モーメントおよびスピン量子数 S が得られる。 以下は Supporting Information の記述である。 1. 常磁性種、内部標準を含んだ溶液を入れた NMR チューブの中に、内部標準だけを含んだ溶液を入れたキャピラリーを入れ、 NMR を測定する。 2. 内部標準のピークのシフト幅 Δν から磁化率 χ (cm 3 g -1 )を 計算する(式1)。 1 (ν 0 : 共鳴周波数、 c : 常磁性種の濃度、 M : 常磁性種のモル質量 ) 3. 磁化率 χ に M を 掛けること で、モル磁化率 χ M (cm 3 mol -1 )を 計算する(式2)。 ...
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