Transition-Metal Catalysts for Methane Dehydroaromatization (Mo, Re, Fe): Activity, Stability, Active Sites, and Carbon Deposits

Yujie Liu, Marita Ćoza, Victor Drozhzhin, Yannis van den Bosch, Lingqian Meng, Rim van de Poll, Emiel J.M. Hensen, Nikolay Kosinov (Corresponding author)

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Samenvatting

The most studied catalysts for methane dehydroaromatization (MDA)─Mo/ZSM-5─are not commercialized yet due to the rapid deactivation and insufficient activity. Catalytic systems based on Fe and Re are potential alternatives to Mo-containing zeolites. Here, we compare the catalytic performance of these catalysts as a function of metal type and its loading in ZSM-5 zeolite. The results show that the catalytic activity decreases in the order of Re/ZSM-5 > Mo/ZSM-5 > Fe/ZSM-5, while the catalyst stability decreases in the opposite order: Fe/ZSM-5 > Mo/ZSM-5 > Re/ZSM-5. The active metal species in the working catalysts were determined by operando X-ray absorption near-edge structure spectroscopy combined with mass spectrometry. We found that Re0 and Fe2+ species are the most likely active species for the catalytic dehydroaromatization of CH4 to aromatics in respective catalysts. Combining the pulse reaction technique with operando thermogravimetry analysis-mass spectrometry experiments, we demonstrate that the length of the induction period strongly correlates to the activity of the catalyst. The longer induction period of the Fe/ZSM-5 catalyst indicates the slow growth of hydrocarbon pool intermediates inside the zeolite pores and thus explains its poor catalytic performance. Finally, both the formation of hydrocarbon pool species and the activity of Fe/ZSM-5 can be improved by increasing the Fe loading, reaction pressure, and space velocity.

Originele taal-2Engels
Pagina's (van-tot)1-10
Aantal pagina's10
TijdschriftACS Catalysis
Volume13
Nummer van het tijdschrift1
DOI's
StatusGepubliceerd - 6 jan. 2023

Bibliografische nota

Publisher Copyright:
© 2022 The Authors. Published by American Chemical Society.

Financiering

Financial support from China Scholarship Council (NO.201806930028) is gratefully acknowledged. We acknowledge the European Synchrotron Radiation Facility and the Diamond Light Source for provision of synchrotron radiation facilities. We thank Dr. Alessandro Longo (ESRF) and Dr. Diego Gianolio (Diamond Light Source) for assistance with XAS experiments.

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