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分子筛中焦炭形成的空间和时间分辨原位光谱:H-ZSM-5和H-SAPO-34上的甲醇制烯烃转化

Space- and time-resolved in-situ spectroscopy on the coke formation in molecular sieves: methanol-to-olefin conversion over H-ZSM-5 and H-SAPO-34.

作者信息

Mores Davide, Stavitski Eli, Kox Marianne H F, Kornatowski Jan, Olsbye Unni, Weckhuysen Bert M

机构信息

Inorganic Chemistry and Catalysis Group, Department of Chemistry, Debye Institute for Nanomaterials Science, Utrecht University, Sorbonnelaan 16, 3584 CA Utrecht, The Netherlands.

出版信息

Chemistry. 2008;14(36):11320-7. doi: 10.1002/chem.200801293.

Abstract

Formation of coke in large H-ZSM-5 and H-SAPO-34 crystals during the methanol-to-olefin (MTO) reaction has been studied in a space- and time-resolved manner. This has been made possible by applying a high-temperature in-situ cell in combination with micro-spectroscopic techniques. The buildup of optically active carbonaceous species allows detection with UV/Vis microscopy, while a confocal fluorescence microscope in an upright configuration visualises the formation of coke molecules and their precursors inside the catalyst grains. In H-ZSM-5, coke is initially formed at the triangular crystal edges, in which straight channel openings reach directly the external crystal surface. At reaction temperatures ranging from 530 to 745 K, two absorption bands at around 415 and 550 nm were detected due to coke or its precursors. Confocal fluorescence microscopy reveals fluorescent carbonaceous species that initially form in the near-surface area and gradually diffuse inwards the crystal in which internal intergrowth boundaries hinder a facile penetration for the more bulky aromatic compounds. In the case of H-SAPO-34 crystals, an absorption band at around 400 nm arises during the reaction. This band grows in intensity with time and then decreases if the reaction is carried out between 530 and 575 K, whereas at higher temperatures its intensity remains steady with time on stream. Formation of the fluorescent species during the course of the reaction is limited to the near-surface region of the H-SAPO-34 crystals, thereby creating diffusion limitations for the coke front moving towards the middle of the crystal during the MTO reaction. The two applied micro-spectroscopic techniques introduced allow us to distinguish between graphite-like coke deposited on the external crystal surface and aromatic species formed inside the zeolite channels. The use of the methods can be extended to a wide variety of catalytic reactions and materials in which carbonaceous deposits are formed.

摘要

已采用空间和时间分辨的方式研究了甲醇制烯烃(MTO)反应过程中大型H-ZSM-5和H-SAPO-34晶体中焦炭的形成。通过将高温原位池与显微光谱技术相结合,实现了这一点。光学活性含碳物种的积累使得可以用紫外/可见显微镜进行检测,而直立配置的共聚焦荧光显微镜则可以观察到催化剂颗粒内部焦炭分子及其前体的形成。在H-ZSM-5中,焦炭最初在三角形晶体边缘形成,其中直通道开口直接通向晶体外部表面。在530至745 K的反应温度下,由于焦炭或其前体,检测到了约415和550 nm处的两个吸收带。共聚焦荧光显微镜显示,荧光含碳物种最初在近表面区域形成,并逐渐向晶体内扩散,其中内部共生边界阻碍了体积较大的芳香族化合物的轻易渗透。对于H-SAPO-34晶体,反应过程中会出现一个约400 nm的吸收带。如果在530至575 K之间进行反应,该吸收带的强度会随时间增加,然后降低,而在较高温度下,其强度随反应时间保持稳定。反应过程中荧光物种的形成仅限于H-SAPO-34晶体的近表面区域,从而在MTO反应过程中对焦炭前沿向晶体中部移动造成了扩散限制。所采用的两种显微光谱技术使我们能够区分沉积在晶体外部表面的类石墨焦炭和在沸石通道内形成的芳香族物种。这些方法的应用可以扩展到形成含碳沉积物的各种催化反应和材料。

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