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首页> 外文期刊>The journal of physical chemistry, C. Nanomaterials and interfaces >Concerted Proton-Transfer Mechanism and Solvation Effects in the HNC/HCN Isomerization on the Surface of Icy Grain Mantles in the Interstellar Medium
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Concerted Proton-Transfer Mechanism and Solvation Effects in the HNC/HCN Isomerization on the Surface of Icy Grain Mantles in the Interstellar Medium

机译:星际介质中冰粒幔表面HNC / HCN异构化过程中的协同质子传递机理和溶剂化作用

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摘要

In order to better understand the isomerization between HNC and HCN on icygrain(or comet nuclei)surfaces in the interstellar medium in connection with a Strecker synthesis route to glycine,B3LYP/6-31+G(d,p)calculations have been carried out on the mechanisms of direct proton transfer(PT),where water molecules play a purely solvating role,and indirect PT,where water molecules participate in a proton relay mechanism.In the direct PT mechanism,a rather high-energy barrier exists for isomerization of HNC to HCN.In the much more important indirect mechanism,a concerted PT process is possible for isomerization in the presence of several water molecules.The calculations show that three water molecules bound to HNC and HCN give rise to a ring reaction significantly favoring the isomerization,a mechanism previously found for this reaction by Gardebien and Sevin(J.Phys.Chem.A 2003,107,3925).Further quite important solvation effects are included in the present work by addition of explicit solvating water molecules,and by a comparison with Polarizable Continuum Model(PCM)solvation.The final calculated free-energy barrier at 50 K is 3.4 kcal/mol for the isomerization of HNC to HCN with three water molecules in a ring acting as a bridge for concerted PT and seven explicit solvating water molecules;PCM solvation of this entire system leads to a further free-energy barrier reduction of 0.8 kcal/mol.The back isomerization of HCN to HNC,however,is unlikely,with an estimated free-energy barrier of 9.5 kcal/mol at 50 K.These results imply that,on icy surfaces in the interstellar medium,the isomerization of HNC to HCN occurs relatively easily,and the implications for the Strecker synthesis of glycine are discussed.
机译:为了更好地理解星际介质中冰晶(或彗核)表面上HNC和HCN之间的异构化,以及与Strecker合成甘氨酸的途径,已进行了B3LYP / 6-31 + G(d,p)计算在直接质子传递(PT)的机制中,水分子起纯溶剂化作用;在间接PT中,水分子参与质子传递机制。在直接PT机理中,存在相当高的能垒用于异构化从HNC到HCN。在更重要的间接机制中,可能存在多个水分子的情况下协同PT异构化过程。计算结果表明,与HNC和HCN结合的三个水分子会产生明显促进异构化的环反应,这是Gardebien和Sevin(J.Phys.Chem.A 2003,107,3925)先前发现的用于该反应的机制。通过添加显式溶剂化物,本研究还包括了非常重要的溶剂化作用。通过与可极化连续体模型(PCM)的溶剂化比较,最终计算出的HNC异构化为HNC时将三个水分子作为桥的HCN异构化为HCN在50 K下的自由能垒为3.4 kcal / mol用于协调的PT和七个明显的溶剂化水分子;整个系统的PCM溶剂化进一步使自由能垒降低0.8 kcal / mol.HCN向HNC的反向异构化可能性不大,估计具有自由能这些结果表明,在星际介质的冰表面上,HNC异构化为HCN相对容易,并且对Strecker合成甘氨酸的意义进行了讨论。结果表明,在50 K时9.5 kcal / mol的分子屏障。

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