光催化
微晶
共轭体系
星团(航天器)
还原(数学)
氧还原
材料科学
氧气
光化学
空位缺陷
化学
化学工程
催化作用
有机化学
结晶学
物理化学
冶金
电化学
计算机科学
复合材料
聚合物
几何学
数学
电极
工程类
程序设计语言
作者
Krishna Samanta,Laxmikanta Mallick,Rahul Ghosh,Biswarup Chakraborty
标识
DOI:10.1002/cctc.202402153
摘要
Abstract An Anderson‐type hetero‐polyoxoanion, [Al(OH) 6 Mo 6 O 18 ] 3− (AlMo 6 ) is conjugated to the polycrystalline TiO 2 matrix (AlMo 6 @TiO 2 ) through multiple [Ti─O─Mo] linkages, characterized by various spectroscopic studies. X‐ray photoelectron spectroscopy (XPS) and electron paramagnetic resonance (EPR) studies reveal high surface oxygen vacancies with dominant Ti 3+ species in the AlMo 6 @TiO 2 . The experimentally determined band gap of 3.11 eV and conduction and valence band potential of −0.84 and 2.27 V (vs NHE), respectively, of AlMo 6 @TiO 2 is ideal to catalyze photochemical CO 2 reduction to CO and CH 4 , with significantly higher activity than bulk anatase TiO 2 . Detailed characterization and photocatalysis data show that despite having a lower lifetime of 0.39 µs for AlMo 6 @TiO 2 than 0.62 µs of bulk anatase TiO 2 , the higher photoreduction of CO 2 to CO by AlMo 6 @TiO 2 is driven by the oxygen vacancies of TiO 2 . However, the use of a 10% H 2 O‐dimethyl sulfoxide mixture leads to a change in the product selectivity to 94% CH 4 . AlMo 6 cluster is used here as a redox‐active and sufficiently bulky anionic cluster to uplift the bands of polycrystalline TiO 2 towards more negative potential, sufficiently higher than CO 2 reduction potential, and induces significant lattice defects, or vacancy sites exposed during photocatalytic CO 2 reduction with comparatively higher photochemical activity than the bulk TiO 2 .
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