Confirmation of 13CO2 photoconversion into
a 13C-product is crucial to produce solar fuel. However,
the total reactant and charge flow during the reaction is complex;
therefore, the role of light during this reaction needs clarification.
Here, we chose Ag–ZrO2 photocatalysts because beginning
from adventitious C, negligible products are formed using them. The
reactants, products, and intermediates at the surface were monitored
via gas chromatography–mass spectrometry and FTIR, whereas
the temperature of Ag was monitored via Debye–Waller factor
obtained by in situ extended X-ray absorption fine structure. With
exposure to 13CO2, H2, and UV–visible
light, 13CO selectively formed, while 8.6% of the 12CO mixed in the product due to the formation of 12C-bicarbonate species from air that exchanged with the 13CO2 gas-phase during a 2 h reaction. By choosing the light
activation wavelength, the CO2 photoconversion contribution
ratio was charge separated at the ZrO2 band gap (λ
< 248 nm): 70%, localized at the Ag surface plasmon resonance (LSPR)
(330 < λ < 580 nm): 28%, and characterized by a thermal
energy of 295 K: 2%. LSPR at the Ag surface was converted to heat
at temperatures of up to 392 K, which provided an efficient supply
of activated H species to the bicarbonate species, combined with separated
electrons and holes above the ZrO2, which generated CO
at a rate of 0.66 μmol h–1 gcat
–1 with approximately zero order kinetics. Photoconversion
of 13CO2 using moisture was also possible. Water
photo-oxidation step above ZrO2 was rate-limited, and the
side reactions that formed H2 above the Ag were successfully
suppressed instead to produce CO via the Mg2+ addition
to trap CO2 at the surface.