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Catalysis Science & Technology
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Journal Name
ARTICLE
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Gan, P. J. Dyson and G. Laurenczy, ReDaOctI.: 1K0i.n10e3t9. /CDa0tCaYl.01L0e8t8t.J,
2009, 98 , 205. d) Y. Zhao, L. Deng , S.-Y. Tang , D.-M. Lai , B.
Liao , Y. Fu and Q.-X. Guo , Energy Fuels, 2011, 25 , 3693.
G. H. Gunasekar, H. Kim and S. Yoon, Sustain. Energy Fuels,
2019, 3, 1042–1047.
Tests with the bare supports proved that conversion was
negligible.
Conclusions
The synthesis of molybdenum carbide by the TPR method using
a CH4/H2 feed was performed successfully over activated carbon
and two high surface area graphites, H200 and H400, of different
graphitic layer dimension. The formed carbide nanoparticles
were between 2.0 and 8.1 nm size which depended on the
surface area and metal loading. Also, the characterization
showed that the carbide phase was influenced by the support.
Accordingly, when activated carbon was used, the Mo2C
phase was obtained mostly exclusively. However, over H400 and
H200 the oxycarbide phase, MoOxCy was also observed. We
explained the differences based on the graphitic layer size. This
is related to the availability of defective carbon which in turn
favours the carburisation. Interestingly, XANES experiments
showed that even under a CH4/H2 atmosphere the main source
of carbon is the support itself. This also implies that smaller
particles, which are in closer contact with the support, are more
easily carburised.
The different molybdenum carbide phase influences the
catalytic performance. The results showed that the Mo2C
phase is more active and selective than the MoOxCy. However,
since MoOxCy is also active on the WGS reaction, the selectivity
to CO2 increases during the reaction. Moreover, Mo2C
supported on activated carbon proved to be stable under
reaction conditions.
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Conflicts of interest
There are no conflicts to declare.
Acknowledgements
We acknowledge financial support from the Spanish Agencia
Estatal de Investigación (AEI) y el Fondo Europeo de Desarrollo
Regional (FEDER), UE (projects CTQ2017-89443-C3-1-R and
CTQ2017-89443-C3-3-R). The ESRF synchrotron is thanked for
granting beamtime at BM23. A.B.Dongil acknowledges financial
support from Fundación General CSIC (Programa ComFuturo).
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