“…The formulation of the emission efficiency in eqs and assumes simple relaxation behavior from a single excited state, even when the transition is the sum of many vibrational modes. The observed emission vibronic-sideband intensities of typical Ru-bpy chromophores are energy dependent ,− and can be effectively modeled by density functional theory (DFT) computations of the configurational mixing of the MLCT/ππ* excited states, and this mixing is correlated with an “extra” energy dependence of k RAD . ,, Consequently, two limiting cases for the photoinduced transition related to the intensity stealing of excited states mixing have been considered in the literature: (a) when a {D, A} system has a strong spin-allowed transition localized on a D or A moiety (e.g., A → A*), it can mix with a weak donor-to-acceptor charge-transfer (DACT) excited state, {D, A} + h ν → {D + , A – }*, thereby enhancing the intensity observed for the DACT transition, and this type of mixing is based on the expression of the molecular model; ,, (b) the emission transitions in phosphorescence require significant mixing between the singlet and T e states through a SOC perturbation ,,− since a pure T e → S 0 transition is strictly spin-forbidden ( M T e ,S 0 = 0) without SOC interactions. The magnitude of the SOC element ( H SOC ) increases approximately as the fourth power of the atomic number ( Z 4 ) and is approximately 3000 times greater for Ru than for C. Furthermore, to ensure that the SOC mixing coefficient is not zero for the T e → S 0 transition, the differences in the T e and S n spin angular momenta ( S⃗ ) must be compensated by the difference in the orbital angular momenta ( L⃗ ) for a spin–orbit operator ( Ĥ SO ∝ S⃗ · L⃗ ).…”