Abstract
An approximate quantitative calculation is given for the effect of spin‐orbit coupling in perturbing the 3A2 state of H2CO. The spin‐orbit coupling mixes the 3A2 state with some higher singlet state, and allows the 3A21A1 transition to have nonvanishing probability. The calculations show that the 3A21A1, np→π2 transition of H2CO should be perturbed principally by the 1A11A1, π1→π2 transition. The bands of the 3A21A1 transition should therefore have the structure of a transition which is allowed by orbital symmetry with an oscillating electronic transition moment along the C–O axis (parallel bands). The oscillator strength, f, is calculated to be f3A21A1≅1.5×10−7 . The natural radiative lifetime τ for the 3A21A1 phosphorescence transition is calculated to be τ≅1×10−2sec . The calculated value for τ is in agreement with the experimental values for the related molecules (CH3)2CO, (C6H5)2CO, and C6H5COCH3, insofar as a comparison can be made. It is further shown that the spin‐orbit perturbation in the π→π* transitions of aromatic hydrocarbons should be about one thousand times less effective than the spin‐orbit perturbation in the n→π* transitions of carbonyl compounds. This is in agreement with the few pieces of experimental data which have been reported thus far.