The negative ion photoelectron spectra of 1,2-dicyanobenzene
(o-DCNB), 1,3-dicyanobenzene (m-DCNB),
and
1,4-dicyanobenzene (p-DCNB) radical anions (DCNB·–), acquired through the computation of Frack-Condon
(FC) factors, are presented. The FC calculations utilize harmonic
frequencies and normal mode vectors derived from density functional
theory at the B3LYP/aug-cc-pVQZ basis set. All the totally symmetric
vibrational modes are treated with Duschinsky rotations to yield neutral
DCNBs in their singlet (So) and lowest triplet (T1) states, following an electron removal from the doublet anionic
ground state. For the So state, the adiabatic electron
affinities (EAs) for o-, m-, and p-DCNB are 1.179, 1.103, and 1.348 eV. The EAs for the lowest
T1 state in o-, m-, and p-DCNB are 4.151, 4.185, and 4.208 eV, resulting in an So–T1 energy difference (ΔE
ST) of 2.973, 3.082, and 2.860 eV. A vibrational analysis
reveals evidence of FC activity involving ring distortion, C–N
bending, and ring CC stretching vibrational progressions in
both the So and T1 states. With the detection
of cyanonaphthalene (C10H7CN) and cyanoindene
(C9H7CN) in the interstellar medium (ISM), our
results highlight the extent to which replacing a single hydrogen
on an aromatic molecule with a cyano group, CN, can alter
the vibrational structure of the molecule/radical anion. As such,
dicyano-polyaromatic hydrocarbons may be reasonably robust in the
ISM, making it appealing to search for them in future interstellar
detection missions.