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Bimetallic nanoparticles were synthesised with either simultaneous
reduction of metal precursors (co-reduction) or the successive re-
duction assisted by hydrogen (hydrogen-sacrificial reduction
method) to produce random alloy and core–shell particles, respec-
tively. The PVP/(Ir+Ni) ratio of 20:1 (molar basis) was used for all
the bimetallic nanoparticles. Three different Ni–Ir alloys with the
molar ratios of Ni/Ir=3:1, Ni/Ir=1:1 and Ni/Ir=1:3 were synthes-
ised by the co-reduction of the metallic precursors. In all cases,
quantities of 0.1 mmol of (Ni+Ir) were used and the same amount
of NaBH4 (0.38 g) was added at 130–1408C. The resulting colloidal
solution obtained was always macroscopically homogeneous and
transparent without any precipitate. As the final Ni/Ir molar ratios
in the g-Al2O3-supported catalysts were found as 1.9:1, 0.9:1 and
1:3, respectively, they are referred as Ni2Ir1, Ni1Ir1 and Ni1Ir3. In
addition to the alloy particles mentioned above, another bimetallic
nanoparticle composition, Ni(core)–Ir(shell) was synthesised (with
the molar ratio of 1:1) using the hydrogen-sacrificial reduction
method, and referred as Ni(c)Ir(s). For the latter combination, Ni
core nanoparticles were synthesised as detailed below. After the
heating time at reflux, colloidal solution was allowed to cool to RT
followed by purging with hydrogen for 1.5 h. This procedure cre-
ates Ni hydride,[40] which further served to reduce Ir and forms an
Ir shell around the preformed Ni nanoparticles. To build an Ir shell,
H2Cl6Ir·xH2O (0.1 mmol) was dissolved in ethylene glycol (ꢀ50 mL)
and added to the mixture of Ni nanoparticles drop by drop. A sy-
ringe pump (Fisher Scientific 01001) was used to transfer Ir solu-
tion to the synthesis flask with a flow rate of approximately
20 mLhÀ1. The synthesis flask was constantly purged with H2
during the addition of Ir and at least one hour afterwards. Each re-
sulting colloidal dispersion was macroscopically homogeneous and
transparent with no precipitate.
were individually counted for 600 s using a 22% relative efficiency
ORTEC hyperpure Ge detector housed in a 10 cm Pb cave. The Ge
detector was connected to a PC-based Aptec multichannel analy-
ser card.
Fresh and calcined supported catalysts were analysed by an Ele-
mentar Vario Micro elemental analyser for CHN percentage.
H2–TPR was performed by using an AutoChem 2950 HP device (Mi-
cromeritics). Quantities of approximately 500 mg of the calcined
catalysts were used for the analysis. Samples were initially reduced
in a 50 mLminÀ1 flow of a mixture of 10% H2 in Ar at T=4008C for
1 h, then cooled to ambient temperature and oxidised in
a 50 mLminÀ1 flow of 10% O2 in He at T=4008C for 1 h. The TPR
profiles were collected with a 10 mLminÀ1 mixture of 10% H2 in Ar
from ambient temperature to 4008C with a heating rate of
108CminÀ1. Peak deconvolution was performed by using Origin
software.
CO2–TPD was performed with the same AutoChem 2950 HP
device. Quantities of approximately 250 mg of the similar calcined
catalysts but with higher metal loading (ꢀ1 wt%) were used for
this study because the Al2O3 also adsorbed CO2. Before CO2 ad-
sorption, samples were initially outgassed in Ar at 3008C for 2 h,
and then reduced by a mixture of 10% H2 in Ar at 4008C for 1 h.
After the reduction pretreatment, the active gas was switched to
He and the temperature was reduced to 508C. A mixture of 3%
CO2 in He was passed through the samples at 508C for 1 h with
the flow of 50 mLminÀ1. Physically adsorbed CO2 was then re-
moved by flushing 50 mLminÀ1 of He at 508C for 1 h. The TPD
spectra were collected by flowing 20 mLminÀ1 He from ambient
temperature to 3008C with a heating rate of 108CminÀ1
.
DRIFTS of adsorbed CO was performed with a Nicolet Nexus670
spectrophotometer, at a resolution of 4 cmÀ1in the range 800–
3000 cmÀ1and averaged over 128 scans. The Ni–Ir nanoparticles
were supported on g-Al2O3 with the higher loading of approxi-
mately 1 wt%. Following the same calcination treatment, that is,
2 h at 4008C in air, catalysts were reduced in the AutoChem 2950
with a flow of 50 mLminÀ1 of 10% H2 in Ar from ambient tempera-
ture to 4008C and kept for 1 h. Subsequently, they were allowed
to cool to RT under a flow of Ar and later a mixture of 3% CO in
He with a flow of 50 mLminÀ1 was passed over the samples for ap-
proximately 45 min. CO-adsorbed catalysts were further treated
with a flow of Ar at RT for approximately 30 min to desorb the
physically adsorbed CO; the DRIFTS spectra of the CO-adsorbed
catalysts were recorded immediately. KBr from Sigma–Aldrich was
dried at approximately 2008C overnight and used for collecting
the background spectra. Samples were also diluted with KBr at the
ratio of approximately 20 wt.% before placing in the DRIFTS cell.
The reflectance spectra of the catalysts were transformed to Kubel-
ka–Munk using the OMNIC software. OMNIC and Origin software
were used for further data processing, visualisation and deconvolu-
tion of the spectra.
All synthesised nanoparticles were supported on pre-dried g-Al2O3
by using acetone to precipitate them.[71] Acetone (ꢀ800 mL) was
added to the suspension of nanoparticles (in colloidal solution)
and g-Al2O3, and it was stirred vigorously for 2 h. Then, the super-
natant was removed from the beaker and the resulting powder
was washed several times with acetone and dried at ambient over-
night to form fresh catalysts, which then were calcined in air at
4008C for 2 h to ensure PVP removal.
Catalyst characterisation
Formation of nanoparticles in the colloidal solution was studied by
UV/Vis spectroscopy by using a Varian Cary 50 Scan UV visible
spectrometer with a 1 cm quartz cell.
TEM images of as-synthesised and supported nanoparticles were
recorded with a JEOL JEM2100 TEM device with a LaB6 filament
operating at 200 kV. The system was equipped with a Gatan GIF
Tridiem energy filter with a 2kꢂ2k digital camera. Samples for TEM
analysis were prepared by placing a drop of the colloidal disper-
sion of nanoparticles onto a carbon-coated copper grid, followed
by the evaporation of the solvent in a vacuum oven at 508C. The
average diameter and the standard deviation were calculated by
counting over 200 particles by using the ImageJ software. In the
case of supported catalysts, the sample (0.1 g) was suspended in
ethanol (5 mL) and dispersed in an ultrasonic bath for approxi-
mately 5 min before placing a drop of the suspension on the TEM
grid.
XPS was performed by using a Kratos Axis 165 X-ray photoelec-
tron spectrometer with a mono AlKa source operating at 15 mA
and 14 kV. The XPS analysis was done on pelletised samples that
were calcined in air at 4008C for 2 h followed by the reduction in
hydrogen at 4008C for 1 h. Background subtraction (Shirley-type),
smoothing and peak fitting were performed by using the CasaXPS
software package. All the core-level spectra were corrected with C
1 s at 284.6 eV.
The loading of the Ni and Ir in the calcined catalysts was deter-
mined by neutron activation analysis at the University of Alberta
SLOWPOKE facility. Samples were irradiated in the nuclear reactor
for 600 s following a decay period of ꢁ24 h. Irradiated samples
ꢀ 2014 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
ChemCatChem 2014, 6, 885 – 894 892