The formation of methane (CH4), formaldehyde (H2CO), ethylene glycol (HOCH2CH2OH), methoxymethanol
(CH3OCH2OH), dimethyl ether (CH3OCH3), and ethanol (CH3CH2OH) upon electron
irradiation of condensed multilayer adsorbates of CH3OH
as a model of cosmic CH3OH ice has been monitored by the
combined use of electron-stimulated and thermal desorption experiments.
The energy-dependent relative yields of all products were measured
between 2.5 and 20 eV, and the reaction mechanisms of product formation
were deduced. The energy dependences of the yields of HOCH2CH2OH, CH3OCH2OH, CH3OCH3, and CH3CH2OH agree closely
with their threshold at the lowest electronic excitation energy of
CH3OH. The formation of these products is consequently
ascribed to the reactions of radicals formed by the dissociation of
neutral electronically excited states and, at higher energy, also
by ionization and subsequent proton transfer to an adjacent CH3OH. These electron–molecule interactions also can contribute
to the nonresonant formation of H2CO and CH4; these latter products are also produced through resonances around
4 eV reported previously from anion electron-stimulated desorption
(ESD) experiments and around 13 eV seen earlier in the energy-dependent
yield of carbon monoxide (CO). The present results constitute the
most complete data set on the energy dependence of product formation
during low-energy electron exposure of condensed CH3OH
so far. They provide a comprehensive picture of the reactions triggered
by electron impact with energies in the range between 2.5 and 20 eV
as representative of low-energy secondary electrons that are released
from condensed material, for instance, under the effect of cosmic
radiation.