ACS Catalysis
Research Article
of the other catalysts were prepared via the same methods with
different quantities of HAuCl4 and Cu(NO3)2 aqueous
solutions.
the catalytic performance at different irradiation wavelengths
(action spectrum experiments). The light intensity of the LED
light sources used for the wavelength-dependent experiments
2
Characterization of Catalysts. The sizes, morphologies,
and compositions of the catalyst samples were characterized by
TEM using a JEOL 2100 transmission electron microscope
equipped with a Gatan Orius SC1000 CCD camera and an
Oxford X-Max EDS instrument. The Au and Cu contents of the
prepared catalysts were determined by EDS technology using
an EDS attachment to an FEI Quanta 200 environmental
scanning electron microscope. Diffuse-reflectance UV/vis (DR-
UV/vis) spectra of the sample powders were examined using a
was 0.2 W/cm , and the light intensity was maintained constant
for each wavelength-dependent experiment. The other reaction
conditions were kept identical with the halogen lamp
photocatalytic reactions. The apparent quantum yield was
calculated as AQY = [(Ylight − Ydark)/(number of incident
photons)] × 100%, where Ylight and Ydark are the number of
products formed under light irradiation and in the dark,
respectively. The number of products formed, Y, was calculated
using the equation Y = y × (moles of reactant) × Avogadro
constant, where y is the product aniline yield for the reaction.
Varian Cary 5000 spectrometer with BaSO as a reference. The
4
light absorption data were normalized with OriginPro 8
software using the normaliziation method “normalize to [0,
ASSOCIATED CONTENT
Supporting Information
■
1]”. The normalized data were plotted against wavelength to
*
S
get the light absorption spectrum of the catalyst. XPS data were
acquired using a Kratos Axis ULTRA X-ray photoelectron
spectrometer incorporating a 165 mm hemispherical electron
energy analyzer. The incident radiation was monochromatic Al
Kα X-rays (1486.6 eV) at 225 W (15 kV, 15 mA). Narrow high-
resolution scans were run with 0.05 eV steps and a 250 ms
dwell time. The base pressure in the analysis chamber was 1.0 ×
Figures S1−S8 and Tables S1−S7 (PDF)
AUTHOR INFORMATION
Notes
■
−
9
8
1
1
0
0
Torr, and during sample analysis the pressure was 1.0 ×
Torr. Peak fitting of the high-resolution data was carried
−
The authors declare no competing financial interest.
out using the CasaXPS software.
Photocatalytic Reactions. A 20 mL Pyrex glass tube was
used as the reaction container, and after the reactants and
catalyst had been added, the tube was sealed with a rubber
septum cap. The reaction mixture was stirred magnetically and
irradiated using a Nelson halogen lamp with a wavelength in
the range 400−800 nm (see Figure S8 in the SI) as the visible-
light source, and the light intensity was measured to be 0.5 W/
ACKNOWLEDGMENTS
■
The authors gratefully acknowledge financial support from the
Australian Research Council (ARC DP110104990 and
DP150102110).
REFERENCES
■
2
cm . The temperature of the reaction system was carefully
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5, and 620 ± 5 nm were used as the light sources to investigate
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ACS Catal. 2016, 6, 1744−1753