The 3-ethynylcyclopentenyl radical
(3ecpr) has been identified
as the carrier of an electronic spectrum with origin at 21792 cm–1 using resonant ionization and laser-induced fluorescence
spectroscopies. The radical was first detected in a toluene discharge
and is most efficiently produced from 1,6-heptadiyne. Overwhelming
spectroscopic and chemical evidence support our diagnosis: (1) the
observed (6.93 eV) and calculated (CCSD(T)/pVQZ) adiabatic
ionization energies are the same; (2) the origin band rotational contour
can be well simulated with calculated rotational constants; (3) convincing
vibrational assignments can be made using computed frequencies; and
(4) the same spectrum was observed in a discharge of 1-ethynylcyclopentanol,
which contains the 3ecpr carbon framework. The π-chromophore
is essentially that of trans-1-vinylpropargyl, a
highly resonance-stabilized C5H5 radical that
persists in conditions relevant to both combustion and circumstellar
atmospheres. We suggest that 3ecpr may be a similarly important radical
warranting inclusion in models of C7H7 chemistry.
It is the second C7H7 isomer with a five-membered
ring yet to be detected, the other being vinylcyclopentadienyl, a
species crucially involved in a recently proposed mechanism of soot
formation (Science, 2018, 361, 6406, 997–1000).
We argue that 3ecpr should be a significant product of H addition
to ethynylcyclopentadiene (C7H6), a known product
of benzyl decomposition. Further, it is plausible that 3ecpr is the
unidentified C7H7 product of sequential addition
of acetylene to propargyl (J. Phys. Chem. Lett.,
2015, 6, 20, 4153–4158) in which 1-vinylpropargyl is an intermediate.
As such, the nC2H2 + C3H3 cascade could represent a facile synthesis of
a substituted five-membered ring in flames and stellar outflows.