ACS Catalysis
Research Article
propylene, which is one of the core commodity chemicals. The
major drawback of the above CO2-based approach is low
propanol selectivity (<4.5%) with respect to C2H4 due to high
catalyst activity for nondesired C2H4 hydrogenation to C2H6. It
is, however, well-documented that the rate of olefin hydro-
genation over supported catalysts with Au NPs can be tuned by
metal loading and average NPs size.13−15 For example, Sermon
et al.14 showed for Au/SiO2 catalysts that the 1-pentene
hydrogenation rate related to overall Au amount decreased with
rising metal loading (0.05 to 5 wt %); the worst hydrogenation-
active catalyst was Au(5 wt %)/SiO2, possessing Au NPs of
about 23 nm. Chou et al.15 systematically investigated micelle-
encapsulated Au NPs supported on TiO2, ZnO, ZrO2, and SiO2
in C3H6 hydrogenation and found that Au/TiO2 with the
smallest Au NPs of 8 nm showed the highest hydrogenation
activity. For liquid-phase cyclohexene hydrogenation over Au/
SiO216 with Au NPs ranging from 10 to 20 nm, the catalyst with
the smallest NPs was the most active one. In addition, our
recent studies on CO2 conversion into propanol in the presence
of C2H4 and H2 established that the nondesired C2H4
hydrogenation to C2H6 over Au/TiO2 catalysts could be
partially suppressed by the usage of promoters like K2O8 or
Cs2O.9 Unfortunately, the conversion of CO2 decreased with
promoter loading, too.
The objective of this study was to elucidate the effects of
support and promoter on the activity and selectivity of
supported Au NPs in the conversion of CO2, C2H4, and H2
into propanol. Our specific aims were (i) to increase propanol
selectivity with respect to ethylene, that is, to reduce
nondesired ethylene hydrogenation to ethane and (ii) to
improve CO2 conversion without significant loss of high
propanol selectivity with respect to this feed component. To
this end, we explored the potential of SiO2-supported catalysts
containing similarly sized (around 5 nm) Au NPs but different
amounts of K for their activity and selectivity in the target
reaction. For comparative purposes, K−Au/TiO2 catalysts
promoted by either potassium nitrate8 or potassium silicate
were also investigated. Fundamentals of CO2 activation were
studied by means of CO2 temperature-programmed desorption
tests and CO2 pulse experiments in the temporal analysis of
products reactor. The latter technique was also applied for
analyzing C2H4 adsorption. To determine the size of Au NPs,
the used catalysts were characterized by high-angle annular dark
field (HAADF) and annular bright field (ABF) scanning
transmission electron microscopy (STEM).
overnight, and calcined in air at 573 K for 4 h. Doping of
calcined samples with K was performed via incipient-wetness
impregnation method with an aqueous solution of KNO3
(>99%, Merck). Hereafter, drying and calcination steps were
repeated yielding XK−Au/SiO2 with ″X″ representing the
particular K weight concentration.
Additionally, two batches of supported catalysts based on
TiO2 anatase (BASF, SBET of 58 m2 g−1) were prepared. They
differed in the source (KNO3 vs K2SiO3) of K and the method
of its deposition on TiO2. For a first batch, Au was initially
loaded onto TiO2 as described in ref 10. Thereafter, Au/TiO2
was incipient-wetness impregnated with a mixture of KNO3 and
K2SiO3 (SiO2/K2O = 2.5:1 wt %, Alfa Aesar) with the portion
of K2SiO3 being 10%, 50%, or 100% gaining an overall K
content of 3 wt %. These titania-supported catalysts were dried
at 353 K overnight, and calcined in static air at 573 K for 4 h.
Such catalysts are abbreviated as XK-YK(Si)-Au/TiO2, where
″X″ and ″Y″ stand for the particular K weight concentration
from KNO3 and K2SiO3, respectively.
To prepare the second batch of catalysts, we first
impregnated TiO2 anatase with K2SiO3 dissolved in concen-
trated ammonia (pH of solution 11−11.5) according to an
incipient-wetness method. The nominal K loading was 1 wt %.
In a next step, the obtained TiO2−K2SiO3 precursor was dried
at 353 K and further impregnated with an aqueous solution of
HAuCl4·xH2O to achieve a loading of Au of 2 wt %. After an
additional drying step, a concentrated ammonia solution was
added to the Au-loaded TiO2−K2SiO3 precursor for an
incipient wetness deposition of Au(OH)3, held impregnated
for 10 min, and washed with water under filtration for chlorine
removal. Hereafter, Au/TiO2−K2SiO3 was dried overnight at
353 K and then doped with K through an incipient-wetness
method using an aqueous solution of KNO3 to obtain 1, 3, and
5 wt % K. After the last doping step, all the titania-supported
catalysts were dried at 353 K overnight and calcined in static air
at 573 K for 4 h. These catalysts were called XK−Au/TiO2−
K2SiO3 where ″X″ stand for the particular K weight
concentration from KNO3. Finally, all as-prepared precursors
were pressed and sieved to yield particles of 250−450 μm.
The weight content of Au and K in the fresh but calcined
catalysts was determined by inductively coupled plasma optical
emission spectrometry (ICP-OES) using a Varian 715 emission
spectrometer.
The Brunauer−Emmet−Teller specific surface areas (SBET
)
were determined from nitrogen adsorption−desorption iso-
therms collected at 77 K on BELSORP-mini II (BEL Japan,
Inc.).
2. EXPERIMENTAL SECTION
2.1. Preparation and Characterization of Au-Contain-
ing Catalysts. K−Au/SiO2 materials with the nominal Au
loading of 2 wt % and different (1−4 wt %) amounts of K were
prepared by sequential deposition−precipitation and incipient
impregnation methods, similar to the procedure for K−Au/
TiO2 catalysts.8 SiO2 (Grade 646, Davisil, SBET of 301 m2 g−1)
was initially calcined in air at 773 K for 8 h. Two grams of
calcined SiO2 were suspended in 200 mL deionized water, and
then the appropriate amount of HAuCl4·xH2O (41.1 wt % Au,
Chempur) was added. The suspension was stirred at 343 K for
1 h and afterward cooled to room temperature. Ammonia (25%
aqueous solution, Roth) used as a reducing agent was added to
the aqueous suspension until a pH value of around 10−10.5
was reached. This pH range was chosen according to the results
of Somodi et al.17 After an additional 10 min of stirring, Au/
SiO2 precursor was filtrated, thoroughly washed, dried at 353 K
The size of Au NPs on the surface of the catalysts was
determined by high-angle annular dark field scanning trans-
mission electron microscopy (HAADF-STEM) employing an
aberration-corrected JEM-ARM200F microscope operated at
200 kV and equipped with a JED-2300 energy-dispersive X-ray
spectrometer (EDXS, JEOL) for elemental analysis. Scanning
transmission electron microscopy (STEM) operations were
done using a Cs-corrector CESCOR (CEOS). Samples were
deposited on a holey-carbon-supported copper grid of mesh
size 300. Particle size distributions of supported Au NPs were
calculated from at least 150 particles with ImageJ software.18
Powder X-ray diffraction (XRD) analysis was carried out
using an X’Pert Pro (Panalytical, Almelo) at the 2θ range of 5−
80° and using a silicon standard. Phase composition of the
samples was identified with the program WINXPow by
3318
ACS Catal. 2016, 6, 3317−3325