Among the species discovered in the
interstellar medium and planetary
atmospheres, a crucial role is played by the so-called “interstellar”
complex organic molecules (iCOMs) because they are the signature of
the increasing molecular complexity in space. Indeed, they may represent
the connection between simple molecules and biochemical species like
amino acids and nucleobases. In particular, HCN and the related CN
radical are the starting points of rich nitrile chemistry. In this
framework, we have undertaken a computational investigation of the
gas-phase reaction mechanisms involving different C2N2H5 radicals and their fragments, stemming from
the addition of the cyano radical to the nitrogen atom of methylamine.
Aiming at exploiting an accurate yet cost-effective protocol, a combination
of CCSD(T)-based composite schemes and density functional theory has
been employed. The exploration of the plausible chemical reaction
channels has led to the identification of 12 different products, as
well as 28 transition states connecting reactants, intermediates,
and products. Aminoacetonitrile (H2NCH2CN),
proposed as an intermediate in the formation of the smallest amino
acid glycine, and the CH2NH2 radical appear
as products energetically accessible under astrophysical conditions.