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Journal of the American Chemical Society
experiments, which indicated a very dynamic H movement even
where Au and Ag have much higher reaction energy for C-C
splitting and are inactive for ethanol decomposition.
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between inter-molecular C-H fragments. Therefore, after the C-C
bond is cleaved, the resulting -CH3 group quickly combines with
an H atom from CHx fragments to form CH4.27 The decomposition
of CD3CH2OH yielded CD4, CD3H and CH2D2 (Figure S15). The
major form of methane was CD3H, suggesting that combining a -
CH3 group with an H atom from -CH2- group is favorable, since an
H atom from the -OH group made a minor contribution to CH4
formation. A relatively large amount of CH2D2 (18%) was
observed, implying that a -CH3 moiety easily dehydrogenated and
recombined with an H atom from the -CH2- group to form CH4
since β-carbon from the -CD3 group is the only source of CH4.
Formation of CD4 suggested that a -CD3 moiety can combine with
a D atom from the -CD3 of a neighboring ethanol, direct evidence
of an inter-molecular reaction. When equal amounts of CD3CD2OD
and CH3CH2OH were used, all forms of methane were detected
(Table 1), again suggesting an inter-molecular reaction. The high
concentration of CH4 compared to CD4 indicates that the
deuteration of the methane produces a primary kinetic isotope
effect (kH/kD = 69.9%/9.9% = 7),28 where CH4 formation is limited
by the combination between –CH3 and the H atom from –CH2-
moiety.
In summary, we report room-temperature liquid-phase
conversion of ethanol into CH4 and CO2 via C-C bond splitting.
Reported results are different from reforming process,1, 6, 8 where
ethanol and water can be easily activated at high
temperature/pressure for H2 and CO2 productions. The reaction
pathways were studied using isotope-labeled ethanol. DFT
calculations in vacuum and liquid conditions suggested that C-C
bond splitting remains mechanistically difficult, but that the
reaction energy for C-C breaking is lowered in liquid compared to
vacuum. This study provides the understanding of breaking C-C
bonds in alcohols or other hydrocarbons via room-temperature
liquid-phase reaction using noble metal nanocatalysts.
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ASSOCIATED CONTENT
Supporting Information
Material synthesis/characterization and DFT calculations are
presented in the Supporting Information. The Supporting
Information is available free of charge on the ACS Publications
website.
AUTHOR INFORMATION
Corresponding Author
ACKNOWLEDGMENT
This work was supported by the National Science Foundation
(CBET–1159662). Research conducted at the Advanced Photon
Source at the Argonne National laboratory and Center for
Functional Nanomaterials at Brookhaven National Laboratory was
sponsored by the U.S. Department of Energy.
Figure 3. DFT calculations conducted in (a) vacuum and (b) liquid ethanol
for the ethanol decomposition. Blue numbers are reaction energies and red
number are activation energies (all in eV).
REFERENCES
Figure 3 shows the DFT calculations of catalytic cycles for
ethanol decomposition on Rh (111) surfaces in vacuum and liquid
conditions. More details are shown in Figure S16-S20. Among
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*CH3 + *OCH2 *CH4 + *CO2), the reaction energy for C-C
breaking (*CH3CH2O *CH3 + *OCH2) is the highest (0.64 eV).
This suggests C-C splitting remains mechanistically difficult
during liquid-phase ethanol decomposition. Notably, reaction
energies of each catalytic step are lowered (or at least comparable)
in liquid compared to in vacuum. Especially the reaction energy for
C-C breaking is significantly lower in liquid (0.64 eV) compared
to in vacuum (1.07 eV). We also modeled C-C breaking in *CH3CO
and *CH2CO (key intermediates during ethanol oxidation19, 29) in
vacuum and liquid conditions. C-C breaking energies in liquid were
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Supporting Information), suggesting ethanol decomposition via C-
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ethanol. This indicates that in the presence of water, ethanol
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(Figure S22), the activities of which follow: Rh ≈ Pt > Ir >> Au ≈
Ag. The reaction energies of C-C splitting on (111) surfaces of
various metal were calculated in vacuum (Figure S23-S26). Three
precursors (*CH3CO, *CH2CO, and *CHCO) were considered,
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