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Fuel
journal homepage: www.elsevier.com/locate/fuel
The effect of lanthanide promoters on NiInAl/SiO
2
catalyst for methanol
synthesis
Anthony R. Richard
a
, Maohong Fan
a,b,
⁎
a
Department of Chemical Engineering, University of Wyoming, Laramie, WY 82071, USA
b
School of Energy Resources, University of Wyoming, Laramie, WY 82071, USA
GRAPHICAL ABSTRACT
ARTICLE INFO
Keywords:
Lanthanides
Rare earth elements
Methanol synthesis
CO2 utilization
Nickel indium catalyst
ABSTRACT
The addition of lanthanides, or rare earth elements, as promoters to NiInAl/SiO
2
methanol synthesis catalysts
was investigated. The promoters studied are the light rare earth elements (La to Gd) and all but La and Ce were
shown to improve methanol synthesis activity. A comparison of the synthesis method for introduction of Pr as a
promoter found that addition during the deposition-precipitation synthesis of the catalyst is superior to incipient
wetness impregnation introduction after synthesis. The heaviest lanthanides tested (Sm, Eu, Gd) showed the
greatest improvement in methanol synthesis activity and selectivity, with a concomitant decrease of CO pro-
duced. The Gd-promoted catalyst showed the greatest increase in methanol synthesis activity at
0.51 mmol g
cat
-1
h
-1
which is a 27% increase over the catalyst with no promoter. Examination of the basic
characteristics of the catalysts by CO
2
TPD and in situ FTIR revealed a negative correlation between basicity and
methanol synthesis activity. FTIR methanol synthesis tests also revealed a larger proportion of the key inter-
mediate, bidentate formate, with the addition of the Gd promoter. STEM micrographs and particle size dis-
tributions show that the incorporation of the Gd promoter results in smaller diameter metallic particles and
higher resistance to sintering. EELS mapping revealed that the location of Ni and Gd correlates well with the
metallic particles observed with STEM, and while the In is also found in these particles, small amounts are also
observed to be dispersed outside of the particles.
https://doi.org/10.1016/j.fuel.2018.02.185
Received 24 December 2017; Received in revised form 24 February 2018; Accepted 28 February 2018
⁎
Corresponding author at: Department of Chemical Engineering, University of Wyoming, Laramie, WY 82071, USA.
E-mail address: mfan@uwyo.edu (M. Fan).
Fuel 222 (2018) 513–522
Available online 23 March 2018
0016-2361/ © 2018 Elsevier Ltd. All rights reserved.
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