Jalbout Abraham F, Abrell Leif, Adamowicz Ludwik, Polt Robin, Apponi A J, Ziurys L M
Instituto de Quimica, Universidad Nacional Autonoma de Mexico, Ciudad Universitaria, Mexico D.F.
Astrobiology. 2007 Jun;7(3):433-42. doi: 10.1089/ast.2006.0083.
Prebiotic possibilities for the synthesis of interstellar ribose through a protic variant of the formose reaction under gas-phase conditions were studied in the absence of any known catalyst. The ion-molecule reaction products, diose and triose, were sought by mass spectrometry, and relevant masses were observed. Ab initio calculations were used to evaluate protic formose mechanism possibilities. A bilateral theoretical and experimental effort yielded a physical model for glycoaldehyde generation whereby a hydronium cation can mediate formaldehyde dimerization followed by covalent bond formation leading to diose and water. These results advance the possibility that ion-molecule reactions between formaldehyde (CH(2)O) and H(3)O(+) lead to formose reaction products and inform us about potential sugar formation processes in interstellar space.
在无任何已知催化剂的情况下,研究了在气相条件下通过质子化形式的福尔摩斯反应合成星际核糖的益生元可能性。通过质谱法寻找离子 - 分子反应产物二糖和三糖,并观察到了相关质量。使用从头算计算来评估质子化福尔摩斯反应机制的可能性。一项双边的理论和实验工作产生了一个用于生成乙醇醛的物理模型,即水合氢离子可以介导甲醛二聚化,随后形成共价键,生成二糖和水。这些结果提高了甲醛(CH₂O)与H₃O⁺之间的离子 - 分子反应导致福尔摩斯反应产物的可能性,并为我们提供了关于星际空间中潜在糖形成过程的信息。