Department of Chemical and Biomolecular Engineering, The University of Melbourne. Parkville 3010, Victoria, Australia.
J Phys Chem A. 2010 Jul 1;114(25):6861-9. doi: 10.1021/jp101279p.
The hydroxyl radical (OH) controls the removal of organic compounds from the troposphere. Atmospheric chemistry models significantly under-predict OH levels in unpolluted environments, implying that they are regenerated via some unknown mechanism(s). This work uses computational chemistry to demonstrate that the photochemical oxidation of alkyl carboxylic acids can efficiently regenerate the hydroxyl radical via unimolecular decomposition of alpha-carboxyalkylperoxy radicals. For acetic acid and propanoic acid the proposed mechanism is predicted to dominate in the unpolluted lower troposphere, and it may also operate to some extent in the mid to upper troposphere. Alkyl carboxylic acids are also predicted to act as a new source of nighttime OH throughout the planetary boundary layer, where OH levels are also under-predicted. The thermodynamic requirements for reactions of this class are discussed, and some candidate OH-reforming molecules particularly relevant to aromatic photooxidation are identified. Adopting a broader perspective, the alpha-carboxyalkyl radical precursors that react with O(2) to form the unstable alpha-carboxyalkylperoxy type radicals are also expected to form during combustion, in the interstellar medium, and from the gamma-irradiation of glycine and related amino acids, and the potential importance of this new chemistry in these environments is discussed. Master equation simulations suggest that alpha-carboxyalkyl + O(2) reactions provide a prompt OH source during the autoignition and combustion of biodiesel and other oxygenated biofuels, where carboxylic acids are formed as early stage oxidation products. Ketene combustion is also thought to proceed via these OH-reforming alpha-carboxyalkyl radicals. The in vivo formation of alpha-carboxyalkylperoxy radicals followed by oxidation to the highly reactive OH radical may induce oxidative stress in the human body, in a process initiated by gamma-rays. Finally, the reaction of ketenes with OH to form alpha-carboxyalkyl radicals, followed by addition of NH(2) or related species, is suggested as a new extraterrestrial pathway to amino acids.
羟基自由基 (OH) 控制着大气中有机化合物的去除。大气化学模型严重低估了未受污染环境中的 OH 水平,这表明它们通过一些未知的机制得以再生。本工作使用计算化学证明,通过α-羧基烷基过氧自由基的单分子分解,烷基羧酸的光化学氧化可以有效地再生羟基自由基。对于乙酸和丙酸,所提出的机制预计将在未受污染的低层大气中占主导地位,并且在中高层大气中也可能在一定程度上起作用。烷基羧酸也被预测为整个行星边界层中夜间 OH 的新来源,而边界层中的 OH 水平也被低估了。讨论了这类反应的热力学要求,并确定了一些与芳香族光氧化特别相关的候选 OH 转化分子。从更广泛的角度来看,与 O(2)反应形成不稳定的α-羧基烷基过氧类型自由基的α-羧基烷基自由基前体也预计会在燃烧过程中、星际介质中以及甘氨酸和相关氨基酸的γ辐照下形成,并且这种新化学在这些环境中的潜在重要性进行了讨论。主方程模拟表明,α-羧基烷基 + O(2) 反应在生物柴油和其他含氧生物燃料的自动点火和燃烧过程中提供了一个即时的 OH 源,其中羧酸作为早期氧化产物形成。烯酮燃烧也被认为是通过这些 OH 转化的α-羧基烷基自由基进行的。α-羧基烷基过氧自由基的体内形成,随后氧化为高反应性的 OH 自由基,可能会在人体中引发氧化应激,这一过程是由γ射线引发的。最后,建议将烯酮与 OH 反应形成α-羧基烷基自由基,然后与 NH(2)或相关物质加成,作为一种新的外星氨基酸形成途径。