A detailed quantum
chemical investigation of a new reaction mechanism
possibly leading to the formation of cyanoketene (NC–CHCO)
in the interstellar medium (ISM) was carried out. Different reaction
channels have been found by the AutoMeKin program, and the structures
and harmonic force fields of the key stationary points have been characterized
at the density functional theory level employing last-generation double-hybrid
functionals. Finally, single-point computations at those geometries
by state-of-the-art composite wave function methods provided accurate
energies for the evaluation of thermochemical and kinetic parameters
in the framework of an Ab Initio Transition State
Theory based Master Equation (AITSTME) strategy. Our results indicate
that the barrier-less association reaction of the formyl radical (HCO•) to the cyanocarbene radical (HCCN) can lead to the
formation of cyanoketene under the harsh conditions of the ISM. Canonical
rate constants computed for temperatures up to 600 K show that the
most abundant product is indeed cyanoketene. The formation of other,
even more stable, species involves higher activation energies and/or
less favorable multi-step processes. Furthermore, to aid the search
of cyanoketene, still undetected in the ISM, its rotational spectrum
was recorded up to 530 GHz. The refined set of spectroscopic constants
obtained in this way allows for spectral predictions from the microwave
to the terahertz region, particularly for the bright b-type transitions,
which can be targeted for the identification of cyanoketene in spectral
line surveys. Despite cyanoketene was already sought without success
in a variety of astronomical sources, we suggest to look for it in
those sources where HCO or HCCN have already been detected, namely,
W3, NGC2024, W51, K3-50, IRC + 2016, and TMC-1.