Resonance-stabilized
radicals are considered as possible intermediates
in the formation of polycyclic aromatic hydrocarbons (PAHs) in interstellar
space. Here, we investigate the fulvenallenyl radical, the most stable
C7H5 isomer by IR/UV ion dip spectroscopy employing
free electron laser radiation in the mid-infrared region between 550
and 1750 cm–1. The radical is generated by pyrolysis
from phthalide. Various jet-cooled reaction products are identified
by their mass-selective IR spectra in the fingerprint region, based
on a comparison with computed spectra. Interestingly, benzyl is present
as a second resonance-stabilized radical. It is connected to fulvenallenyl
by a sequence of two H atom losses or additions. Among the identified
aromatic hydrocarbons are toluene and styrene, as well as polycyclic
molecules, such as indene, naphthalene, fluorene and phenanthrene.
Mechanisms for the formation of PAH from C7H5 have already been suggested in previous computational work. In particular,
the radical/radical reaction of two fulvenallenyl radicals provides
an efficient route to phenanthrene in one bimolecular step and might
be relevant for PAH formation under astrochemical conditions.