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Electronic structure and spectra of the RbAr van der Waals system including spin-orbit interaction

机译:RbAr van der Waals系统的电子结构和光谱,包括自旋轨道相互作用

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The potential energy curves and spectroscopic constants of the ground and excited states of the RbAr van der Waals system have been determined using a one-electron pseudopotential approach. This technique is used to replace the effect of the Rb + core and the electron-Ar interactions by effective potentials. The core-core interaction for Rb +Ar was incorporated using the accurate CCSD(T) potential of Hickling et al. [ Hickling, H. L.; Viehland, L. A.; Shepherd, D. T.; Soldán, P.; Lee, E. P. F.; Wright, T. G. Phys. Chem. Chem. Phys. 2004, 6, 4233-4239 ]. This model reduces the number of active electrons of the RbAr van der Waals systems to just the single valence electron, permitting the use of very large basis sets for the Rb and Ar atoms. Using this approach, the potential energy curves of the ground and excited states dissociating into Rb(5s, 5p, 4d, 6s, 6p, 6d, and 7s) + Ar are calculated at the SCF level. Spin-orbit interaction was also considered within a semiempirical scheme for the states dissociating into Rb(5p) and Rb(6p). Spectroscopic constants are derived and compared with the available theoretical and experimental data. Such comparisons for RbAr show very good agreement for the ground and the first excited states. Furthermore, we have predicted the B ~2∑ + _(1/2) ← X ~2∑ ~+, A ~2π _(1/2) ← X ~2∑ ~+, A ~2π _(3/2) ← X ~2∑ ~+, A ~2π _(3/2) ← X ~2∑ ~+, 5 ~2∑ ~+ ← X ~2∑ ~+, 3 ~2π _(1/2) ← X ~2∑ ~+, and 3 ~2π _(3/2) ← X ~2∑ ~+ absorption spectra.
机译:RbAr van der Waals系统的基态和激发态的势能曲线和光谱常数已使用单电子pseudo势方法确定。该技术用于用有效电势代替Rb +核和电子-Ar相互作用的作用。使用Hickling等人的准确CCSD(T)势能结合了Rb + Ar的核-核相互作用。 [Hickling,H. L .; Viehland,L. A .;牧羊人D. P.Soldán; Lee E.P.F .; Wright,T。G. Phys。化学化学物理2004,6,4233-4239]。该模型将RbAr van der Waals系统的活性电子数减少到仅一个价电子,从而允许对Rb和Ar原子使用非常大的基集。使用这种方法,在SCF级别上计算了分解为Rb(5s,5p,4d,6s,6p,6d和7s)+ Ar的基态和激发态的势能曲线。在半经验方案中还考虑了自旋轨道的相互作用,使状态解离为Rb(5p)和Rb(6p)。得出光谱常数,并将其与可用的理论和实验数据进行比较。对于RbAr的这种比较显示出对于基态和最初的激发态具有很好的一致性。此外,我们已经预测到B〜2∑ + _(1/2)←X〜2∑〜+,A〜2π_(1/2)←X〜2∑〜+,A〜2π_(3/2 )←X〜2∑〜+,A〜2π_(3/2)←X〜2∑〜+,5〜2∑〜+←X〜2∑〜+,3〜2π_(1/2)← X〜2∑〜+和3〜2π_(3/2)←X〜2∑〜+吸收光谱。

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