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原位紫外/可见微光谱和一组互补的分子模拟方法鉴定沸石催化反应中的中间体。

Identification of intermediates in zeolite-catalyzed reactions by in situ UV/Vis microspectroscopy and a complementary set of molecular simulations.

机构信息

Center for Molecular Modeling (CMM), Ghent University, Technologiepark 903, 9052 Zwijnaarde (Belgium), QCMM-alliance, Ghent-Brussels (Belgium).

出版信息

Chemistry. 2013 Dec 2;19(49):16595-606. doi: 10.1002/chem.201301965. Epub 2013 Nov 5.

Abstract

The optical absorption properties of (poly)aromatic hydrocarbons occluded in a nanoporous environment were investigated by theoretical and experimental methods. The carbonaceous species are an essential part of a working catalyst for the methanol-to-olefins (MTO) process. In situ UV/Vis microscopy measurements on methanol conversion over the acidic solid catalysts H-SAPO-34 and H-SSZ-13 revealed the growth of various broad absorption bands around 400, 480, and 580 nm. The cationic nature of the involved species was determined by interaction of ammonia with the methanol-treated samples. To determine which organic species contribute to the various bands, a systematic series of aromatics was analyzed by means of time-dependent density functional theory (TDDFT) calculations. Static gas-phase simulations revealed the influence of structurally different hydrocarbons on the absorption spectra, whereas the influence of the zeolitic framework was examined by using supramolecular models within a quantum mechanics/molecular mechanics framework. To fully understand the origin of the main absorption peaks, a molecular dynamics (MD) study on the organic species trapped in the inorganic host was essential. During such simulation the flexibility is fully taken into account and the effect on the UV/Vis spectra is determined by performing TDDFT calculations on various snapshots of the MD run. This procedure allows an energy absorption scale to be provided and the various absorption bands determined from in situ UV/Vis spectra to be assigned to structurally different species.

摘要

通过理论和实验方法研究了嵌在纳米多孔环境中的(聚)芳烃的光吸收特性。碳质物种是甲醇制烯烃(MTO)过程中有效催化剂的重要组成部分。在酸性固体催化剂 H-SAPO-34 和 H-SSZ-13 上进行的甲醇转化的原位 UV/Vis 显微镜测量揭示了在 400、480 和 580nm 左右生长的各种宽吸收带。所涉及物种的阳离子性质通过氨与甲醇处理样品的相互作用来确定。为了确定哪些有机物种导致了各种带,通过时间相关密度泛函理论(TDDFT)计算对一系列芳烃进行了系统分析。静态气相模拟揭示了结构不同的碳氢化合物对吸收光谱的影响,而沸石骨架的影响则通过在量子力学/分子力学框架内使用超分子模型来检查。为了完全理解主要吸收峰的起源,必须对被困在无机主体中的有机物种进行分子动力学(MD)研究。在这种模拟中,充分考虑了灵活性,并通过对 MD 运行的各种快照进行 TDDFT 计算来确定对 UV/Vis 光谱的影响。该程序允许提供能量吸收范围,并将从原位 UV/Vis 光谱确定的各种吸收带分配给结构不同的物种。

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