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Are isomers of the vinyl cyanide ion missing links for interstellarpyrimidine formation?

机译:氰基乙烯基离子的异构体是否缺少星际嘧啶间形成的联系?

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In the interstellar medium (ISM) there are many regions where the formation of molecules iskinetically driven rather than thermochemically, which can lead to the formation of many isomerseven though some may be fairly higher in energy relative to the molecular global minimum. Recentlaboratory experiments where noble gas cations are reacted with pyrimidine favored the formation of C_3H_3N~+, but the molecular structure(s) of this fragment was not determined. Microscopicreversibility means that pyrimidine could form under interstellar conditions should the required C_3H_3N~+reactant be detected in the ISM.Hence could a strong candidate forinvolvement in the formation of heterocyclic biomolecules such as pyrimidine in the ISM. In this study, we have investigated the low energy isomers of the acrylonitrile ion (C_3H_3N~+) using densityfunctional theory as well as high levels of ab initio theory, namely, the singles and doublescoupled-cluster theory that includes a perturbational correction for connected triple excitations,denoted as CCSD(T). An automated stochastic search procedure, Kick, has been employed to find isomers on the ground state doublet potential energy surface. Several new structures, along with allthe previously reported minima, have been found. The global minimum H_2CCCNH~+is energetically much lower than either H_2CC(H)CN~+, the acrylonitrile ion, or HCC(NCH~+, most likelyintermediate of the reaction between HCCH~+and HCN. These isomers are connected to the global minimum via several transition states and intermediates. The results indicate that not only the globalminimum but also several higher energy isomers of the C_3H_3N~+ion could be important in interstellar pyrimidine formation. The isomeric molecules have the necessary CCNC backboneneeded for the reaction with HCN to form the cyclic pyrimidine framework. The structural and rotational parameters of all the isomers studied in this work have been predicted at the CCSD(T)level of theory with the anticipation that it will expedite their laboratory as well as astronomicalidentification.
机译:在星际介质(ISM)中,有许多区域是通过分子动力学而不是通过热化学方法来驱动分子形成的,这可能导致形成许多异构体,即使其中某些异构体的能量可能比分子整体最小值还高。最近的实验室实验中,稀有气体阳离子与嘧啶反应,促进了C_3H_3N〜+的形成,但未确定该片段的分子结构。微观可逆性意味着只要在ISM中检测到所需的C_3H_3N〜+反应物,嘧啶就可能在星际条件下形成,因此可能成为ISM中嘧啶等杂环生物分子形成的有力候选者。在这项研究中,我们使用密度泛函理论和高水平的从头算理论,即单和双偶合簇理论,其中包括对连接三元体的扰动校正,研究了丙烯腈离子的低能异构体(C_3H_3N〜+)激发,表示为CCSD(T)。已使用自动随机搜索程序Kick在基态二重态势能表面上查找异构体。已经发现了几种新结构,以及所有先前报道的最小值。 H_2CCCNH〜+的整体最小值在能量上远低于H_2CC(H)CN〜+,丙烯腈离子或HCC(NCH〜+),这很可能是HCCH〜+与HCN之间反应的中间产物。结果表明,不仅C_3H_3N〜+离子的整体最小值,而且C_3H_3N〜+离子的多个高能异构体在星状嘧啶的形成中也很重要,这些异构分子具有与HCN反应生成CCCN所需的主链。在CCSD(T)的理论水平上预测了这项工作中研究的所有异构体的结构和旋转参数,并预期将加速其实验室研究和天文鉴定。

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