Computational Studies
of CO<sub>2</sub> Activation
via Photochemical Reactions with Reduced Sulfur Compounds
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Abstract
Reactions between CO<sub>2</sub> and reduced sulfur compounds
(RSC),
H<sub>2</sub>S and CH<sub>3</sub>SH, were investigated using ground
and excited state density functional theory (DFT) and coupled cluster
(CC) methods to explore possible RSC oxidation mechanisms and CO<sub>2</sub> activation mechanisms in the atmospheric environment. Ground
electronic state calculations at the CR-CC(2,3)/6-311+G(2df,2p)//CAM-B3LYP/6-311+G(2df,2p)
level show proton transfer as a limiting step in the reduction of
CO<sub>2</sub> with activation energies of 49.64 and 47.70 kcal/mol,
respectively, for H<sub>2</sub>S and CH<sub>3</sub>SH. On the first
excited state surface, CR-EOMCC(2,3)/6-311+G(2df,2p)//CAM-B3LYP/6-311+G(2df,2p)
calculations reveal that energies of <250 nm are needed to form
H<sub>2</sub>S–CO<sub>2</sub> and CH<sub>3</sub>SH–CO<sub>2</sub> complexes allowing facile hydrogen atom transfer. Once excited,
all reaction intermediates and transition states are downhill energetically
showing either C–H or C–S bond formation in the excited
state whereas only C–S bond formation was found in the ground
state. Environmental implications of these data are discussed with
a focus on tropospheric reactions between CO<sub>2</sub> and RSC,
as well as potential for carbon sequestration using photocatalysis