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Electronic spectroscopy of carbon chains (C2n+1, n=7-10) of astrophysical importance. II. Quantum dynamics

机译:碳链的电子光谱(C2N + 1,N = 7-10)的天体物理重要性。 II。 量子动态

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In continuation with Paper I [S. R. Reddy et al., J. Chem. Phys. 151, 054303 (2019)], the vibronic structure and dynamics of the (1)Sigma(+)(u) electronic state of C-15, C-17, C-19, and C-21 chains in the coupled manifold of (1)Sigma(+)(u)-(1)Pi(g)-(1)Pi(u)-(1)Sigma(+)(g) electronic states have been investigated in this paper. The model vibronic Hamiltonian developed through extensive ab initio quantum chemistry calculations in Paper I is employed, and first principles nuclear dynamics calculations are carried out to obtain the photoabsorption band of the (1)Sigma(+)(u) electronic state. Both time-independent and time-dependent quantum mechanical calculations are carried out to precisely locate the vibrational levels, assign them with the progression of vibrational modes, and elucidate the impact of both Renner-Teller and pseudo-Renner-Teller couplings on them. The nonradiative decay of the (1)Sigma(+)(u) electronic state is studied, and it is found that the decay rate is comparable with the prediction made for them to be qualified as a carrier of diffuse interstellar bands in the literature. The theoretical results are found to be in good accord with the available experimental results. Published under license by AIP Publishing.
机译:在与纸I [S.延续R. Reddy等人,J。化学式物理。 151,054303(2019)]中,电子振动结构和所述(1)西格玛(+)的动力学(u)的C-15,C-17,C-19,和电子状态C-21链中的连接歧管(1)西格玛(+)(U) - (1)PI(克) - (1)PI(U) - (1)西格玛(+)(克)的电子态已在本文中进行了研究。通过广泛的AB在造纸我开发初始量子化学计算的模型的电子振动哈密顿采用,以及第一原则核动力学计算被执行,以获得(1)西格玛(+)的光吸收带(u)的电子状态。这两个时间独立和时间相关的量子力学计算都进行了精确定位的振动水平,振动模式的发展将它们分配,并阐明两者伦纳 - 泰勒和他们的伪雷纳 - 泰勒耦合的影响。所述(1)西格玛(+)(u)的电子状态的非辐射衰变进行了研究,并且发现,该衰减率是用由对它们进行限定为在文献中漫星际频带的载波的预测相媲美。理论计算结果被发现是在良好的符合现有的实验结果。通过AIP发布在许可证下发布。

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