Chirped-pulse rotational spectroscopy in a quasi-uniform
flow has
been used to investigate the reaction dynamics of a multichannel radical–radical
reaction of relevance to planetary atmospheres and combustion. In
this work, the NO + propargyl (C3H3) reaction
was found to yield six product channels containing eight detected
species. These products and their branching fractions (%), are as
follows: HCN (50), HCNO (18), CH2CN (12), CH3CN (7.4), HC3N (6.2), HNC (2.3), CH2CO (1.3),
HCO (1.8). The results are discussed in light of previous unimolecular
photodissociation studies of isoxazole and prior potential energy
surface calculations of the NO + C3H3 system.
The results also show that the product branching is strongly influenced
by the excess energy of the reactant radicals. The implications of
the title reaction to the planetary atmospheres, particularly to Titan,
are discussed.