A Computational Study of a Prebiotic Synthesis of D-Riboflavin (Vitamin B2)

Nigel Aylward
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Abstract

Ab initio applied computing is used to determine the viability of a plausible mechanism for the formation of riboflavin from planetary and interstellar gases that contain the necessary essential elements. The immutable laws of chemical thermodynamics and kinetics enable the intermediates in the synthesis to be characterized and the activation energies to be established. The gases propyne, cyanogen, carbon monoxide, and hydrogen are invoked in a synthesis of the isoalloxazine precursor of the vitamin riboflavin (Vitamin B2), whilst the additional presence of hydrogen cyanide enables the surface-catalyzed, photochemically activated synthesis of a D-ribitylamine requiring the magnesium metalloporphyrin catalyst. These two molecules then bond in a Sn2 reaction to form the final vitamin structure. The reactions have been shown to be feasible from the overall enthalpy changes in the ZKE approximation at the HF and MP2 /6-31G* level and with acceptable activation energies.
益生元合成d -核黄素(维生素B2)的计算研究
从头算应用计算用于确定从含有必要基本元素的行星和星际气体形成核黄素的合理机制的可行性。化学热力学和动力学的永恒规律使合成过程中的中间体得以表征,活化能得以确定。在合成维生素核黄素(维生素B2)的异alloxazine前体时,会用到丙烯、氰、一氧化碳和氢等气体,而氰化氢的额外存在使得d -核糖胺的表面催化、光化学激活合成需要金属卟啉镁催化剂。然后这两个分子在Sn2反应中结合形成最终的维生素结构。在HF和MP2 /6-31G*水平上,从ZKE近似的总焓变来看,反应是可行的,并且具有可接受的活化能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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