The radiative lifetimes of the b 1Σ + and a 1Δ states of O 2, S 2 and SO have been evaluated by perturbation expansions including 3Σ g −, 1Δ g, 1Σ g +, 1Π g, 3Π g states for the homonuclear systems and 3Σ − (2), 1Δ, 1Σ + (2), 1Π (2), 3Π (2), 3Σ + states for SO; all wavefunctions are MRD CI expansions up to 5000 terms. The mixing coefficients are obtained from the spin-orbit operator in the Breit-Pauli form evaluating all one- and two-particle terms explicitly. In O 2 and S 2 the radiative lifetime of the b 1Σ g + state is found to be largely determined by the spin-contributions to the magnetic moment in the magnetic dipole operator. The calculated value of 11.65 s for O 2 is in excellent agreement with the measured value of 12 s; the calculations predict a lifetime of 3.4 s for b 1Σ g + in S 2. The calculated lifetime corresponding to the b 1Σ g + −a 1Δ g transition is 720 s in good accord with the experimental intensity determination (400 s within a factor of two). The intensity for the a 1Δ g −X 3Σ g − transition is dominated by the orbital angular momentum term in the magnetic-dipole operator and arises from 1Δ g − 1Π g and X 3Σ g − − 3Π g transitions present in the perturbed X 3Σ − and a 1Δ g wavefunctions. Calculated values are τ(O 2) = 5400 s relative to a measured value of 3900 s, and τ = 350 s for S 2 as a prediction. The absence of the inversion favors electric (rather than magnetic) dipole processes in SO. The b 1Σ + −X 3Σ − transition borrows its intensity predominantly from terms connecting b 1Σ + −2 1Σ + and X 3Σ − −2 3Σ − which occur as perturbers in the pure spin wavefunctions. The calculated b 1Σ + lifetime is 13.6 ms in fair accord with the recently measured 7 ± 2 ms. For τ (a 1Δ) the calculations predict intensity borrowing from A 3Π−X 3Σ − and C 3Π−X 3Σ − as well as 1Δ− 1Π and 1Δ−2 1Π dipole transitions resulting in a value of 450 ms. The decrease in lifetime from the first- to the second-row molecules is quantitatively demonstrated to arise from increased spin-orbit interaction, while a different mechanism is responsible for the change in b 1Σ + lifetimes from homonuclear to heteronuclear systems. Finally, all calculations demonstrate that spin-forbidden radiative transition probabilities can be obtained quite effectively by modern-day quantum chemical calculations.
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