Abstract
The structures of phenylcyclopropane (1+•) and cumene (2+•) cation radicals were calculated using both CASSCF and B3LYP computational methods. Both methods predict that 1+• adopts a delocalized, bisected structure and that the barrier to phenyl group rotation is substantial (11−14 kcal/mol). In contrast, the spin and charge in 2+• is largely localized in the phenyl ring and there is no strongly preferred ground state conformation. The CASPT2 method was used to predict the electronic spectra of 1+• and 2+•. The large differences in the spectra of 1+• and 2+• can be traced to significant σ−π interaction in 1+•. The results are rationalized in terms of a simple valence bond configuration mixing model. In general, the calculated transition energies were in good accord with the experimental values; however, the relative UV−vis peak intensities for 1+• were not well reproduced if a static structure was assumed. Better agreement was obtained by taking into account libration of the phenyl group in 1+•.
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