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distribution, particle density and photoabsorption between
2
Au(0.5)/TiO (P25) prepared by CPH and that prepared by
3
g
PH. At least one of those differences is attributable to the
drastic change in the reaction order with respect to light
intensity. We think that the use of colloidal Au particles and
deposition on the TiO
are important for the non-linear photocatalytic reaction
over CPH-Au(0.5)/TiO (P25) even under weak photoirradiation.
Two-photon absorption induced by SPR of Au nanoparticles in
CPH-Au(0.5)/TiO (P25) might account for the non-linearity,
although we have no clear mechanism for the two-photon
absorption. We are now conducting various control experiments
to clarify the key factor in the non-linear catalytic reaction and to
clarify the possibility of two-photon or step-wise two-photon
2
surface without change in particle size
2
2
Fig. 4 Double logarithm plots of the light intensity of visible light and the
reaction rate of evolution of CO
prepared by PH.
2 2
from formic acid over Au(0.5)/TiO (P25)
Under the conditions of intense light irradiation, the reaction induced photocatalytic reaction.
rate tends to be saturated. Interestingly, the rate in the present
This work was partly supported by a Grant-in-Aid for Scientific
reaction system increased with increase in light intensity, Research (no. 23560935) from the Ministry of Education, Culture,
indicating that the reaction order in the present system Sports, Science, and Technology (MEXT) of Japan and by the
was larger than unity with respect to light intensity. Double Cooperative Research Program of the Catalysis Research Center,
logarithm plots of the light intensity of visible light and the Hokkaido University (grant # 10A0006 and 12B1006).
2
reaction rate of Au(0.5)/TiO (P25) are shown in Fig. 3(c). Linear
correlations between them were observed, and the slope of the
plots that corresponded to the reaction order with respect to
References
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2
catalytic reaction under irradiation with light of different
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2
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This journal is c The Royal Society of Chemistry 2013
Chem. Commun., 2013, 49, 3419--3421 3421