Mrugała Felicja
Institute of Physics, Nicolaus Copernicus University, Grudziadzka 5, PL 87-100 Toruń, Poland.
J Chem Phys. 2008 Aug 14;129(6):064314. doi: 10.1063/1.2948389.
Extensive calculations of energies and lifetimes of vibronic and rovibronic states of the CO(2+) dication are performed using the electronic energy potentials and spin-orbit couplings published recently by Sedivcova et al. [J. Chem. Phys. 124, 214303 (2006)] and by Eland et al. [J. Phys. B 37, 3197 (2004)]. Siegert quantization, bound-continuum configuration mixing, two-potential, and semiclassical methods are exploited in the calculations. Lifetimes for predissociation and tunneling, varying over a wide range, are determined, demonstrating a very good agreement between results yielded by the different methods. Dependence of the calculated predissociation characteristics (level widths and shifts) on the individual potentials and couplings is analyzed. The potentials of Sedivcova et al., especially the repulsive potential of the (3)Sigma(-) state, are found insufficiently accurate in the medium range of the internuclear distance to be useful in simulations of the decay of the lowest vibronic states of the ion, X (3)Pi(v = 0,1) and a (1)Sigma(+)(v = 0,1). Combining the potentials of Eland et al. with the SO couplings of Sedivcova et al. is demonstrated to provide the best description of metastability of the ion so far. Purely vibronic models constructed in this way give lifetimes in a reasonable agreement with all existing experimental values and estimates. The largest deviations, tau(expt)/tau(calc) approximately 20, occur in the X (3)Pi(v = 1,2) cases. Strong evidence is provided that accounting for rotational motion of nuclei, spin-uncoupling perturbations, and diagonal spin-orbit couplings can reduce these deviations substantially, approximately ten times. The predissociation lifetimes of the rovibronic states A (3)Sigma(0,1)(+)(Jv) are predicted to be, with no exception, more than 100 times shorter than radiative lifetimes of these states.
利用Sedivcova等人[《化学物理杂志》124, 214303 (2006)]以及Eland等人[《物理学杂志B》37, 3197 (2004)]最近发表的电子能量势和自旋 - 轨道耦合,对CO(2+)二价阳离子的振转电子态和振转振动态的能量及寿命进行了广泛计算。计算中采用了西格特量子化、束缚 - 连续体组态混合、双势以及半经典方法。确定了预解离和隧穿的寿命,其变化范围很广,不同方法得到的结果显示出非常好的一致性。分析了计算得到的预解离特征(能级宽度和位移)对各个势和耦合的依赖性。发现Sedivcova等人的势,特别是(3)Σ(-)态的排斥势,在核间距的中等范围内不够精确,无法用于模拟离子最低振转电子态X (3)Π(v = 0,1)和a (1)Σ+(v = 0,1)的衰变。结果表明,将Eland等人的势与Sedivcova等人的自旋 - 轨道耦合相结合,能提供目前对该离子亚稳性的最佳描述。以这种方式构建的纯振转电子模型给出的寿命与所有现有实验值和估计值合理相符。最大偏差,即τ(expt)/τ(calc)约为20,出现在X (3)Π(v = 1,2)的情况中。有强有力的证据表明,考虑原子核的转动运动、自旋解耦微扰和对角自旋 - 轨道耦合可以大幅减小这些偏差,约为十倍。预计振转振动态A (3)Σ(0,1)+(J v)的预解离寿命无一例外地比这些态的辐射寿命短100倍以上。