2018
DOI: 10.1063/1674-0068/31/cjcp1707137
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Bimetallic RuM (M=Co, Ni) Alloy NPs Supported on MIL-110(Al): Synergetic Catalysis in Hydrolytic Dehydrogenation of Ammonia Borane

Abstract: By adjusting various Ru/M (M=Co, Ni) molar ratios, a series of highly dispersed bimetallic RuM alloy nanoparticles (NPs) anchored on MIL-110(Al) have been successfully prepared via a conventional impregnation-reduction method. And they are first used as heterogeneous catalysts for the dehydrogenation reaction of AB at room temperature. The results reveal that the as-prepared Ru 1 Co 1 @MIL-110 and Ru 1 Ni 1 @MIL-110 exhibit the highest catalytic activities in different RuCo and RuNi molar ratios, respectively.… Show more

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Cited by 6 publications
(2 citation statements)
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“…And the ones at 282.9 and 280.7 eV are designated to Ru 0 3d 3/2 and Ru 0 3d 5/2 , respectively. , The other peaks appearing at 284.3 and 281.5 eV correspond to Ru n + 3d 3/2 and Ru n + 3d 5/2 , respectively. Meanwhile, the characteristic peaks of Ru 3p 3/2 and Ru 3p 1/2 are located at 459.0 and 481.3 eV in the Ru 3p XPS spectrum (Figure d), respectively. Figure e reveals that the binding energies of Ni 2p 3/2 and Ni 2p 1/2 are appeared at 852.6 and 870.0 eV, respectively. The two satellite peaks centered on 858.3 and 876.2 eV belong to Ni 2p 3/2 and Ni 2p 1/2 , respectively, which suggests the existence of Ni n + species such as Ni­(OH) 2 and NiO. , The formation of Ru n + and Ni n + species presumably occurs within the sample preparation procedure for XPS measurements, or might result from the part oxidation of RuNi NPs when being exposed in air.…”
Section: Resultsmentioning
confidence: 90%
“…And the ones at 282.9 and 280.7 eV are designated to Ru 0 3d 3/2 and Ru 0 3d 5/2 , respectively. , The other peaks appearing at 284.3 and 281.5 eV correspond to Ru n + 3d 3/2 and Ru n + 3d 5/2 , respectively. Meanwhile, the characteristic peaks of Ru 3p 3/2 and Ru 3p 1/2 are located at 459.0 and 481.3 eV in the Ru 3p XPS spectrum (Figure d), respectively. Figure e reveals that the binding energies of Ni 2p 3/2 and Ni 2p 1/2 are appeared at 852.6 and 870.0 eV, respectively. The two satellite peaks centered on 858.3 and 876.2 eV belong to Ni 2p 3/2 and Ni 2p 1/2 , respectively, which suggests the existence of Ni n + species such as Ni­(OH) 2 and NiO. , The formation of Ru n + and Ni n + species presumably occurs within the sample preparation procedure for XPS measurements, or might result from the part oxidation of RuNi NPs when being exposed in air.…”
Section: Resultsmentioning
confidence: 90%
“…For this reason, most of the reported CoRu alloy NPs synthesis protocols rely on the impregnation of metal precursors into the support materials and then following reduction of the metal precursors at high temperature. [24][25][26][27][28][29][30][31][32][33][34][35][36] These synthesis protocols yielded polydisperse CoRu NPs with lack of composition control and proof of alloy formation. In this regard, an appropriate method, especially colloidal synthesis method, is needed to prepare CoRu alloy NPs with a monodisperse size distribution and composition control.…”
Section: Introductionmentioning
confidence: 99%