CHEMSUSCHEM
FULL PAPERS
The idea of a carbanion formation by the deprotonation of
the methyl group was considered previously by Iglesia and
Gines,[30] albeit from an adsorbed aldehyde. In their study, the
catalyst was a basic oxide (MgCeOx) modified with Cu and K,
and they used 12C2H5OH/13C2H4O reactant mixtures to establish
that condensation reactions can proceed by the direct reaction
of ethanol without the intermediate formation of gas-phase
acetaldehyde. This means that acetaldehyde condensation may
occur and that ethanol direct condensation contributes to the
formation of the products. Besides, they discussed that the
condensation reactions become easier than dehydrogenation
in presence of a metal (e.g., Cu) as the metal helps to remove
the hydrogen as H2.
Table 2. Alcohol adsorption, reaction and TS energies for the process
that leads to the dehydrogenation of ethanol and methanol on Mg10O10
and for the formation of a carbanion by methyl deprotonation in ethano-
l.[a]
Alcohol/site
Adsorption energy
DE[b]
[kcalmolꢀ1
Barrier[b]
[kcalmolꢀ1
]
[kcalmolꢀ1
]
]
Dehydrogenation
EtOH/Mg3C
EtOH/O3C
MeOH/O3C
MeOH/Mg3C
39.5
23.9
25.1
40.4
38.1 (ꢀ1.4)
29.4 (5.5)
37.0 (11.9)
45.9 (5.5)
44.7 (5.2)
40.4 (16.5)
44.5 (19.4)
51.4 (11.0)
Carbanion formation
EtOH/Mg3C
EtOH/O3C
31.3 (ꢀ8.2)
33.4 (ꢀ6.1)
36.4 (12.5)
36.7 (12.8)
The suggestion of carbanion formation on the MgO surface
rationalises several experimental observations, the simplest
one of which is the production of ethylene. We have located
two TS that lead from the Mg3C-adsorbed carbanion to ethyl-
ene and dissociated water (see Figure 9 for the reactant/TS
structures) with fairly low barrier heights (3.7 and 6.5 kcal
molꢀ1). Such a finding places the barrier to be surmounted
during the carbanion formation plus dehydration sequence at
4.8 kcalmolꢀ1 below the barrier that leads to acetaldehyde
plus H2. Thus, the dehydration of ethanol is a competitive pro-
cess compared to its dehydrogenation even onto the purely
basic MgO. Besides, the carbanion normal mode at n˜ =
1165 cmꢀ1 also helps to assign the IR feature at n˜ =1143 cmꢀ1,
the evolution of which is in line with the reactivity expected
from such species (vide supra, DRIFTS Section and Figure S12,
which show the simulated IR spectrum of the carbanion). Simi-
larly, the position of the two peaks around n˜ =1220 cmꢀ1 in
the spectrum shown in Figure S12 correlates well with the lo-
cation of a shoulder that appears and then disappears in the
DRIFT spectrum upon increasing the temperature. Notably, the
relative intensities in the n˜ =1143–1220 cmꢀ1 region are not re-
produced well by the calculations. We consider that this find-
ing is most likely because the shoulder modes involve the dis-
placement of the proton on MgO that interacts directly with
the anionic carbon atom; the effect of such motion on the mo-
lecular dipole may be estimated improperly by DFT due to of
shortcomings in the description of electronic correlation. In-
stead, the lack of any feature in the DRIFT spectra around n˜ =
1380 cmꢀ1 (Figure S12), a mode connected to the wagging of
OH-bearing CH2 in the carbanion, remains for the moment un-
clear.
[a] The zero of the energy for the processes is assumed to be the ad-
sorbed alcohol with the OH dissociated. [b] In parentheses, there are en-
ergetic quantities that refer to the gas-phase alcohols plus Mg10O10 as re-
actants.
should be considered as active thanks to the high temperature
(4008C) employed during the reaction, and the Mg3C site is
likely to produce more aldehydes, comparatively, thanks to the
lower barrier from the feed reactants.
Enol formation
The enolic form of acetaldehyde would be important if the C4
formation proceeded through the aldolic pathway, and DFT
calculations indicate that C4 formation on Mg3C should release
energy (2 kcalmolꢀ1) and require a low barrier to be surmount-
ed (6.6 kcalmolꢀ1; see Figure 7 for the optimised structures). It
is thus likely that a fast equilibrium may exist between the two
molecules.
Carbanion formation
The basic MgO surface sites may cleave a CꢀH bond hetero-
lythically in the ethanol methyl group, and our calculations
(Table 2 and Figure 8) indicate that such a process generates
a carbanion 31.3 and 36.4 kcalmolꢀ1 above the adsorbed etha-
nol in the vicinity of the Mg3C and O3C sites, respectively. De-
protonation close to the Mg3C site generates a product that is
6.8 kcalmolꢀ1 lower in energy than acetaldehyde plus ad-
sorbed H2 compared to MgO/gaseous ethanol; the TS barriers
for such processes also have the same order of energy. The
carbanion produced close to the O3C site, instead, is higher by
7.0 kcalmolꢀ1 than acetaldehyde/adsorbed H2, although the TS
barriers have the same order as that close to Mg3C. Notably,
the barrier for carbanion formation near O3C is just 0.3 kcal
molꢀ1 above the energetic requirement for the reaction.
With the quantitative results discussed, it is possible to draw
a partial conclusion with respect to the importance of the al-
dolic path toward C4 formation on MgO. The higher energetic
cost to be paid to produce two molecules of acetaldehyde
compared to a single carbanionic species or a carbanion and
an acetaldehyde ought to make the surface concentration of
the acetaldehyde/enol pair substantially less than that of the
carbanion/acetaldehyde couple (or the carbanion/ethanol pair,
vide infra). In turn, this suggests that the aldolic pathway is
less likely than the one that involves the carbanion. Additional
arguments against the aldolic scheme come from the fact that
the adsorbed aldol lies substantially higher in energy than the
adsorbed 1,3-BDO and that our DFT calculations predict the al-
The data reported in Table 2 suggest that both Mg3C and
O3C sites may produce the two intermediates, albeit with dif-
ferent activities. In fact, the global energy profiles suggest that
carbanion formation on the Mg3C site ought to be the most
likely process, followed by ethanol dehydrogenation on the
same site and carbanion formation on O3C.
ꢀ 2014 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
ChemSusChem 0000, 00, 1 – 13
&
6
&
ÞÞ
These are not the final page numbers!