Sekiguchi Osamu, Uggerud Einar
Mass Spectrometry Laboratory and Centre for Theoretical and Computational Chemistry (CTCC), Department of Chemistry, University of Oslo , P.O.B. 1033, Blindern, N-0315 Oslo, Norway.
J Phys Chem A. 2013 Nov 7;117(44):11293-6. doi: 10.1021/jp4053715. Epub 2013 Oct 28.
From gas phase reactivity studies employing tandem mass spectrometry, the unimolecular dissociation of the corresponding base of glycolaldehyde has been probed under conditions of collisional activation. Three reactions were observed (in order of decreasing abundance): loss of CO, CH2O, and loss of H2. Detailed reaction mechanisms for each of the three reactions were obtained by quantum chemical calculations, and the reaction characteristics and energetics were found to be in good agreement with experimental observations. The relevance of these findings to the formose reaction and possible interstellar formation of carbohydrates from formaldehyde is discussed. It is concluded that the critical C-C bond forming reaction between two formaldehyde molecules to give the glycoladehyde is unlikely to occur in the gas phase via a route involving the free formyl anion, thereby precluding a key pathway for interstellar formation of carbohydrates. However, an alternative formation reaction is suggested.
通过采用串联质谱的气相反应性研究,在碰撞活化条件下对乙醇醛相应碱的单分子解离进行了探究。观察到三个反应(按丰度递减顺序):CO的损失、CH₂O的损失以及H₂的损失。通过量子化学计算获得了这三个反应各自的详细反应机理,并且发现反应特征和能量学与实验观察结果高度吻合。讨论了这些发现与甲醛聚糖反应以及星际中由甲醛形成碳水化合物的可能关系。得出的结论是,两个甲醛分子之间形成关键C-C键生成乙醇醛的反应不太可能在气相中通过涉及游离甲酰阴离子的途径发生,从而排除了星际形成碳水化合物的一条关键途径。然而,提出了一种替代的形成反应。