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the TDS spectra at m/z = 31 and 45. This ratio is characteristic
of ethanol, as verified by leaking the pure compound into the
chamber. The desorption temperature agrees with that of
pure ethanol (see Figure SI1 in the Supporting Information).
Together, this supports that ethanol is in fact produced.
Low-energy electrons can thus drive the formation of
ethanol in mixed films of C2H4 and H2O at cryogenic
temperature. As for the electron-induced hydroamination,[5,6]
ionization of one of the reactants removes the activation
barrier for the reaction. The formation of ethanol thus
proceeds under conditions that are fundamentally different
from those of technical processes for the production of
ethanol by hydration of C2H4. These processes require high
temperatures, high partial pressures, and a catalyst.[8] This
suggests that the described approach to control adduct
formation may also allow for an atom-efficient synthesis of
other carbon structures containing heteroatoms.
5 eV.[13] In clusters, EA is observed at slightly different
energies, but again not below about 6 eV.[14] However,
nondissociative EA to C2H4 proceeds around 1.5 eV.[15]
Therefore, EA to C2H4 to yield a radical anion C2H4CÀ must
trigger the formation of ethanol at low E0 values. This
provides, at the same time, the first example of an electron-
induced synthesis controlled by a nondissociative EA process.
The range of E0 values observed for this process compares
well with the broadening of a similar EA process in
condensed N2,[16,17] thus supporting our conclusion.
Neither in films of pure C2H4, nor in mixtures of C2H4 and
NH3,[6] did we observe formation of any products at such low
E0 values. This observation points to a key role of H2O in the
reaction observed here, which can be explained by its acidic
protons. Radical anions are typically basic species.[18] The
transient radical anion C2H4CÀ formed by EA to C2H4 can
accept a proton donated by H2O to form an ethyl radical
(C2H5C). In contrast, in aprotic media the radical anion can
only relax through autodetachment of the captured electron,
which is a relaxation channel in all EA processes.[3] We
propose that this proton transfer triggers the complete
sequence of reactions shown in Scheme 2.
Support for the proposed reaction mechanism can be
derived from a thorough analysis of the side products. At
E0 values above the ionization threshold, electron irradiation
of condensed C2H4 produces a variety of hydrocarbons,
including ethane (C2H6), butane (C4H10), butene (C4H8),
butadiene (C4H6),[6] and acetylene (C2H2, see Figure SI2).
Among the C4 hydrocarbons, the C2H4 dimer butene is the
dominant product at E0 = 15 eV.[6] This, together with elec-
tron-stimulated desorption (see Figure SI2), contributes to
the loss of C2H4 during irradiation, as seen in Figure 1. In
contrast, ethane and butane are the predominant products in
the EA regime. Significant contributions of butene and
butadiene can be excluded based on the mass peaks seen by
TDS (see Figure SI3). Furthermore, butane is only formed in
the presence of H2O (see Figure SI4). Together, these findings
strongly support the scenario depicted in Scheme 2.
The intermediate reactive species proposed in Schemes 1
and 2 cannot be monitored directly, although their contribu-
tion to the reactions can be inferred from the product yields as
a function of sample thickness (Figure 3). Anions resulting
from EA are short-lived species that can decay by loss of the
excess electron.[3] This process is enhanced in the vicinity of
a metal surface to which the electron can be transferred.[19]
The opposite process, namely transfer of an electron from the
surface can neutralize cationic intermediates. The probability
of such quenching processes depends on the distance between
the ions and the surface.[19]
In the case of ethylamine,[5,6] the reaction occurred only at
E0 values above the ionization threshold of C2H4 and NH3. To
confirm that electron impact ionization also drives the
formation of ethanol, we have measured the dependence of
ethanol yield on the E0 value. The ionization thresholds of
H2O and C2H4 in the gas phase are 12.6 eV and 10.5 eV,
respectively.[9] In the condensed phase, polarization forces can
lower such thresholds by up to 2 eV.[10] The continuous
increase in product yield with E0 above about 8 eV confirms
an ionization-driven reaction. Surprisingly, however, the
yields of ethanol also increase considerably as the E0 values
decrease below 6 eV (Figure 2).
At E0 values well below the ionization threshold, electron
attachment (EA) to molecules can occur. In the gas phase, the
resulting molecular radical anions usually decay into an anion
and a radical, a process named dissociative electron attach-
ment (DEA).[3,4] However, in condensed phase where polar-
ization forces stabilize the charge, the radical anion may also
survive.[3,4] As neutral excitation processes are absent below
roughly 4 eV in both C2H4 and H2O,[11] such anionic processes
must be responsible for the ethanol yield at low E0 values.
DEA processes for H2O in the gas phase occur around
7 eV, 9 eV, and 11 eV[12] and thus above the range of E0 values
concerned here. No production of OHC radicals occurs below
At E0 values above but near the ionization threshold,
a radical cation initiates product formation. In very thin
layers, quenching of this species by the nearby metal surface
inhibits product formation, as shown here for ethanol, ethane,
and butane (Figure 3, top). At E0 = 3 eV, the formation of
ethane and butane follows the same trend (Figure 3, bottom),
thereby pointing again to quenching by the metal surface. In
both cases, neutralization by quenching occurs before the
intermediate radical ion can react with an adjacent molecule.
However, the production of ethanol at low E0 values only
Figure 2. Dependence of ethanol yields on electron energy (E0) as
represented by the integrated TDS peak areas at m/z=31 obtained
from 30 monolayer (ML) films of a 1:1 mixture of C2H4 and H2O after
electron exposures of 600 mCcmÀ2. The increase above 8 eV is attrib-
uted to a reaction initiated by electron impact ionization, while the
ethanol formation below 6 eV is driven by an electron attachment
process to C2H4.
ꢀ 2015 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
Angew. Chem. Int. Ed. 2015, 54, 4397 –4400