Hechtfischer U, Rostas J, Lange M, Linkemann J, Schwalm D, Wester R, Wolf A, Zajfman D
Max-Planck-Institut für Kernphysik, Heidelberg, Germany.
J Chem Phys. 2007 Nov 28;127(20):204304. doi: 10.1063/1.2800004.
We have measured the photodissociation spectrum of CH(+) and CD(+) molecular ions, stored as fast (MeV) ion beams in the heavy-ion storage ring TSR. Several b (3)Sigma(-)-a (3)Pi bands were observed as strong resonances because a large fraction of the ions in the metastable a (3)Pi(v=0) state were pumped to b (3)Sigma(-) levels and predissociated via the c (3)Sigma(+) state into C(+) and H(D) fragments. From a rotational analysis of the 2-0, 3-0, and 4-0 bands in CH(+) and the 3-0 and 4-0 bands in CD(+), we derive spectroscopic constants for these levels and also revise a previous analysis of the 0-0 and 1-0 bands in CH(+). Combining all data delivers new, significantly adjusted equilibrium constants for the b (3)Sigma(-) and a (3)Pi electronic states. Apart from the spectroscopic analysis, we estimate the predissociation rates of the upper b (3)Sigma(-) vibrational levels in CH(+) and compare them to a model. For the initial rovibrational distribution of the stored metastable CH(+) molecules, the data indicate a faster vibrational cooling than derived before, and rotational cooling at a rate similar to the X (1)Sigma(+) ground state. New aspects of the spin-forbidden a (3)Pi-X (1)Sigma(+) radiative decay are discussed. Finally, we predict b (3)Sigma(-)-a (3)Pi absorption and a (3)Pi-X (1)Sigma(+) emission lines through which CH(+) in the metastable a (3)Pi(v=0) state might be detectable in astrophysical environments.
我们测量了存储在重离子存储环TSR中作为快速(兆电子伏特)离子束的CH(+)和CD(+)分子离子的光解离光谱。观察到几个b (3)Σ⁻-a (3)Π带作为强共振,因为处于亚稳态a (3)Π(v = 0)态的大部分离子被泵浦到b (3)Σ⁻能级,并通过c (3)Σ⁺态预解离为C(+)和H(D)碎片。通过对CH(+)中的2-0、3-0和4-0带以及CD(+)中的3-0和4-0带进行转动分析,我们得出了这些能级的光谱常数,并对之前对CH(+)中0-0和1-0带的分析进行了修正。综合所有数据,得到了b (3)Σ⁻和a (3)Π电子态新的、显著调整后的平衡常数。除了光谱分析,我们估计了CH(+)中较高b (3)Σ⁻振动态的预解离速率,并将其与一个模型进行比较。对于存储的亚稳态CH(+)分子的初始振转分布,数据表明振动冷却比之前推导的更快,转动冷却速率与X (1)Σ⁺基态相似。讨论了自旋禁戒的a (3)Π-X (1)Σ⁺辐射衰变的新方面。最后,我们预测了b (3)Σ⁻-a (3)Π吸收线和a (3)Π-X (1)Σ⁺发射线,通过这些线在天体物理环境中可能检测到处于亚稳态a (3)Π(v = 0)态的CH(+)。