Theoretical Study of the Radiative Lifetime for the Spin-forbidden Transition $X^{1}\Sigma^{+}_{*}<- a^{3}\Sigma^{+}_{u}$ in $He2^{4}$

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1988

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Ohio State University

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Using Ab Initio State Averaged MCSCF Plus CI Methods Chemical Research, Development, and Engineering Center Aberdeen Proving Ground, MD 21010-5423 The radiative lifetime for the a3Σu+ state in neutral He2 was calculated including spin-orbit (SO) interactions between the a3Σ1+ and 1Πu manifold of states, and the repulsive ground state X1Σg and the 3Πg manifold. The SO interactions are treated through first-order perturbation theory wherein the first-order corrections to the wavefunctions are calculated directly by solving a set of linear equations (representing the first-order perturbation expression) involving SO matrix elements between the zeroth-order X1Σg+ or a3ΣU+ wavefunctions, and the list of Configuration State Functions generated by a second-order CI for the states of 3Πg or 1Πu symmetries, respectively (1). This partially alleviates the problem of solving explicitly for many eigenstates of the 3Πg or 1Πu symmetries. The results show a rapidly changing electric transition dipole moment over the bound region of the a3Σu+, i.e. r(HeHe)=1.5 to 4.0 bohr. A vibrational analysis gives the lifetime of the v-O level of a3Σu+ to be around 18 secs, which is consistent with a recent experimental estimate of 10 secs (v-?) as a lower bound.

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1 D. R. Yarkeny, J. Chem. Phys. 86, 1642 (1987); and references therein.


Author Institution: US Army Ballistic Research Laboratory, SLCBR-IB-I; Department of Chemistry, The Johns Hopkins University; Lawrence Livermore National Laboratory, The Johns Hopkins University

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