Cyanoacetylene (HCCCN), the first member
of the cyanopolyyne
family (HC
n
N, where n = 3, 5, 7, ...), is of particular interest in astrochemistry being
ubiquitous in space (molecular clouds, solar-type protostars, protoplanetary
disks, circumstellar envelopes, and external galaxies) and also relatively
abundant. It is also abundant in the upper atmosphere of Titan and
comets. Since oxygen is the third most abundant element in space,
after hydrogen and helium, the reaction O + HCCCN can be of relevance
in the chemistry of extraterrestrial environments. Despite that, scarce
information exists not only on the reactions of oxygen atoms with
cyanoacetylene but with nitriles in general. Here, we report on a
combined experimental and theoretical investigation of the reactions
of cyanoacetylene with both ground 3P and excited 1D atomic oxygen and provide detailed information on the primary
reaction products, their branching fractions (BFs), and the overall
reaction mechanisms. More specifically, the reactions of O(3P, 1D) with HCCCN(X1Σ+) have been investigated under single-collision conditions by the
crossed molecular beams scattering method with mass spectrometric
detection and time-of-flight analysis at the collision energy, E
c, of 31.1 kJ/mol. From product angular and
time-of-flight distributions, we have identified the primary reaction
products and determined their branching fractions (BFs). Theoretical
calculations of the relevant triplet and singlet potential energy
surfaces (PESs) were performed to assist the interpretation of the
experimental results and clarify the reaction mechanism. Adiabatic
statistical calculations of product BFs for the decomposition of the
main triplet and singlet intermediates have also been carried out.
Merging together the experimental and theoretical results, we conclude
that the O(3P) reaction is characterized by a minor adiabatic
channel leading to OCCCN (cyanoketyl) + H (experimental BF = 0.10
± 0.05), while the dominant channel (BF = 0.90 ± 0.05) occurs
via intersystem crossing to the underlying singlet PES and leads to
formation of 1HCCN (cyanomethylene) + CO. The O(1D) reaction is characterized by the same two channels, with the relative
CO/H yield being slightly larger. Considering the recorded reactive
signal and the calculated entrance barrier, we estimate that the rate
coefficient for reaction O(3P) + HC3N at 300
K is in the 10–12 cm3 molec–1 s–1 range. Our results are expected to be useful
to improve astrochemical and photochemical models. In addition, they
are also relevant in combustion chemistry, because the thermal decomposition
of pyrrolic and pyridinic structures present in fuel-bound nitrogen
generates many nitrogen-bearing compounds, including cyanoacetylene.