Full Papers
vation capacity of the materials determined in our previous
mixture was heated to reflux with moderate agitation for 3 h. Hy-
drolysis was performed by the addition of the deionized water. The
gel obtained was aged for 10 h. The samples were dried under
[
37]
À1
work:
zero for Au/Al O , 0.18 mol mol
for Au/CeO ,
2
3
O
Au
2
À1
À1
0.48 mol mol
for Au/Ce(10)-Al, and 0.68 mol mol
Au
for
O
Au
O
À3
vacuum (ꢀ10 torr) at 1008C for 12 h then heated to 4508C
Au/Ce(30)-Al (details are presented in the Supporting Informa-
tion and Figure S9). The amount of adsorbed oxygen may be
considered as the measure of the relative content of (Au–ceria
vacancy) active sites on the catalyst surface.
under N and kept at this temperature for 12 h. Finally, the samples
2
were treated in O at 6508C for 4 h for the decomposition of or-
2
ganic residuals. Nanostructured alumina was prepared by the same
sol–gel method described above without the addition of the
cerium compound. Commercial CeO2 (Alfa-Aesar) was used as
a support as well. The mixed oxide supports were encoded as
Ce(X)-Al and Au/Ce(X)-Al, respectively, in which X (10 or 30) indi-
cates the ceria content (10 or 30 wt%).
Within the mechanism accepted currently for the oxidative
esterification of primary alcohols, the first reaction step in-
volves the dehydrogenation of the alcohol into the aldehyde
followed by the formation of a hemiacetal from the aldehyde
[
11,25,26,39]
and alcohol.
Finally, the dehydrogenation of the hemi-
Au (calculated as 3 wt%) was supported by deposition–precipita-
tion using urea as a precipitation agent according to the proce-
dure developed in Ref. [37]. The support (4.0 g) was added to an
acetal gives the ester. Thus, the introduction of ceria into alu-
mina facilitates the oxygen activation to improve the per-
formance of AuNPs in these oxidation processes because of
the better accessibility of active oxygen species in the Au–ceria
interfacial area. A specific Au–ceria interaction results in the in-
À3
aqueous solution (400 mL) of HAuCl4 (1.6ꢂ10 m) and urea
(
0.42m). The initial pH of the solution was ꢀ2. The suspension was
stirred intensively at 808C for 4 h and then filtered. The solid mate-
rial was washed with ammonium hydroxide (25.0m) for 30 min.
Then samples were washed with water until pH 7, filtered, and
dried at RT for 24 h. Finally, samples were treated in H or O with
[
40]
crease in oxygen mobility, which can also contribute to the
enhanced activity of materials that contain Au supported on
ceria compared to that on alumina. The negative effect of the
2
2
a continuous temperature increase from 50–3508C with a ramp
À1
catalyst pretreatment in H can be explained, at least for the
rate of 208Cmin . The resulting materials were used in the catalyt-
2
ceria-containing materials, by the partial reduction of ceria,
which could affect the capacity of the material to oxygen acti-
vation by increasing the OÀsupport bonding energy.
ic tests.
Catalyst characterization
Conclusions
The chemical composition of the Au samples was determined by
ICP-AES by using a Varian Liberty 110 ICP Emission Spectrometer.
In a typical procedure, the sample (30 mg) was dissolved in a mix-
ture of concentrated H SO , HCl, and HNO (20 mL, H SO /HCl/
Au nanoparticles supported on the Ce–Al mixed oxides pre-
pared by a sol–gel technique are more active in the liquid-
phase aerobic oxidative esterification of benzyl alcohol and
benzaldehyde than Au supported on single cerium or alumi-
num oxides. The reactions occur in methanol solutions in the
absence of any auxiliary base and give methyl benzoate as the
main product. High turnover numbers of up to 19000 reflect
the high stability of the catalysts, which can be reused. The
2
4
3
2
4
HNO =6:6:3, v/v) and heated to 1508C.
3
Specific surface areas were determined using the BET method by
N thermal adsorption measurements by using a Gemini 2600 Mi-
2
cromeritics instrument. Before the analysis, samples were heated in
an Ar flow at 3508C for 1 h. The pore distribution was evaluated
using N adsorption by using a TriStar II Micromeritics unit. Before
2
thermal pretreatment in O resulted in more active catalysts
2
the analysis, samples were heated under vacuum at 3508C for 12 h
to eliminate support impurities and traces of adsorbed water.
than pretreatment in H ; however, the product distributions
2
were similar for the two sets of catalysts. The remarkable syn-
ergetic effect between ceria and alumina may be explained by
the enhanced oxygen storage capacity of the materials pre-
pared from mixed oxides compared to neat alumina and ceria.
The order of the catalytic activity (Au/Al O <Au/CeO <Au/
The qualitative and quantitative analysis of the acid sites in the
supports was performed by IR spectroscopy using pyridine as
[36,42]
a probe molecule as described in detail previously.
The adsorp-
tion of pyridine and the measurement of FTIR spectra were per-
formed at 1008C. The pyridine desorbed at 250, 350, and 4508C
corresponds to weak, medium, and strong acid sites, respective-
2
3
2
Ce(10)-Al<Au/Ce(30)-Al) correlates well with the results of the
oxygen activation capacity of the materials. Thus, the introduc-
tion of ceria into alumina facilitates oxygen activation by Au
nanoparticles and improves their performance in the oxidation
processes strongly.
[42]
À1
ly. Spectral bands at n˜ =1545 and 1450 cm , which correspond
to Brønsted and Lewis acid sites, respectively, were analyzed.
TEM was performed by using a JEOL 2010 microscope. The sample
was dispersed in isopropanol and dropped onto a copper grid
coated with a carbon film. To determine the mean diameter of Au
particles, more than 150 particles were chosen. UV/Visible diffuse
reflectance spectra (UV/Vis DRS) were recorded at RT by using
a Varian Cary 300 scan spectrophotometer equipped with a stan-
Experimental Section
Catalyst preparation
[37]
dard diffuse reflectance unit as described previously. XPS meas-
urements were performed by using a Kratos AXIS 165 spectrome-
ter using monochromatic AlKa radiation (hv=1486.58 eV) and
a fixed analyzer pass energy of 20 eV. All measured BEs refer to the
C1s line of adventitious carbon at BE=284.8 eV. Spectrum decon-
volution was performed with background estimation using the
Nanostructured Ce–Al mixed oxides with different contents of ceria
(
10 and 30 wt%) were prepared by a sol–gel method using
[41]
organometallic precursors as described previously. A solution of
cerium(III) 2,4-pentanedionate hydrate (Alfa-Aesar) in ethanol with
moderate agitation was added to a mixture of aluminum sec-but-
oxide (Alfa-Aesar) in 2-methyl-2,4-pentanediol (Alfa-Aesar), and the
[43]
Shirley algorithm. XRD analysis was performed by using a Philips
&
ChemCatChem 0000, 00, 0 – 0
6
ꢁ 0000 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
ÝÝ These are not the final page numbers!