One of the most spectacular yet unsolved problems for the ICÑ A-band photodissociation is the non-statistical spin-rotation F 1 = N + 1/2 and F 2 = N − 1/2 populations for each rotation level N of the CN fragment. The F 1 /F 2 population difference function f(N) exhibits strong N and λ dependences with an oscillatory behavior. Such details were found to critically depend on the number of open-channel product states, namely, whether both I ( 2 P 3/2 ) and I ( 2 P 1/2 ) are energetically available or not as the dissociation partner. First, in the asymptotic region, the exchange and dipole-quadrupole inter-fragment interactions were studied in detail. Then, as the diabatic basis, we took the appropriate symmetry adapted products of the electronic and rotational wavefunctions for the F 1 and F 2 levels at the dissociation limits. We found that the adiabatic Hamiltonian exhibits Rosen-Zener-Demkov type nonadiabatic transitions reflecting the switch between the exchange interaction and the small but finite spin-rotation interaction within CN at the asymptotic region. This non-crossing type nonadiabatic transition occurs with the probability 1/2, that is, at the diabatic limit through a sudden switch of the quantization axis for CN spin S from the dissociation axis to the CN rotation axis N. We have derived semiclassical formulae for f(N) and the orientation parameters with a two-state model including the 3A 0 and 4A 0 electronic states, and with a four-state model including the 3A 0 through 6A 0 electronic states. These two kinds of interfering models explain general features of the F 1 and F 2 level populations observed by Zare's group and Hall's group, respectively.It is known that the ground state of the I atom has j = 3/2, thus yields the non-zero quadrupole moment due to the non-spherical charge distribution, while the spin-orbit excited state has j = 1/2, WWW.C-CHEM.ORG
FULL PAPERWiley Online Library J. Comput. Chem. 2019, 40, 482-499 485 the space-fixed (SF) Z 0 axis is taken as the propagation direction for circularly polarized light (Fig. 2). Then, we focus on the orientation of the SF total angular momentum of photofragment CN. This orientation is defined asHere, J Z 0 M SF J is the space-fixed Z 0 component of the total angular momentum CN, and ρ J ð Þ M SF J M SF J is the relative population observed in the level M SF J and is normalized as P M SF J ρ J ð Þ M SF J M SF J