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Experimental and Theoretical Study of Reactions of OH Radicals with Hexenols: An Evaluation of the Relative Importance of the H-Abstraction Reaction Channel

机译:OH自由基与己烯醇反应的实验和理论研究:H抽象反应通道相对重要性的评价

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摘要

C6 hexenols are one of the most significant groups of volatile organic compounds with biogenic emissions. The lack of corresponding kinetic parameters and product information on their oxidation reactions will result in incomplete atmospheric chemical mechanisms and models. In this paper, experimental and theoretical studies are reported for the reactions of OH radicals with a series of C6 hexenols, (Z)-2-hexen-1-ol, (Z)-3-hexen-1-ol, (Z)-4-hexen-1-ol, (E)-2- hexen-1-ol, (E)-3-hexen-1-ol, and (E)-4-hexen-1-ol, at 298 K and 1.01 × 10~5 Pa. The corresponding rate constants were 8.53 ± 1.36, 10.1 ± 1.6, 7.86 ± 1.30, 8.08 ± 1.33, 9.10 ± 1.50, and 7.14 ± 1.20 (in units of 10~(-11) cm~3 molecule~(-1) s~(-1)), respectively, measured by gas chromatography with a flame ionization detector (GC-FID), using a relative technique. Theoretical calculations concerning the OH-addition and H-abstraction reaction channels were also performed for these reactions to further understand the reaction mechanism and the relative importance of the H-abstraction reaction. By contrast to previously reported results, the H-abstraction channel is a non-negligible reaction channel for reactions of OH radicals with these hexenols. The rate constants of the H-abstraction channel are comparable with those for the OH-addition channel and contribute >20% for most of the studied alcohols, even >50% for (E)-3-hexen-1-ol. Thus, H-abstraction channels may have an important role in the reactions of these alcohols with OH radicals and must be considered in certain atmospheric chemical mechanisms and models.
机译:C6己烯醇是具有生物成因排放的最重要的挥发性有机化合物之一。缺乏相应的动力学参数和有关其氧化反应的产物信息将导致大气化学机理和模型不完整。本文报道了OH自由基与一系列C6己烯醇(Z)-2-hexen-1-ol,(Z)-3-hexen-1-ol,(Z)反应的实验和理论研究在298 K下的-4-hexen-1-ol,(E)-2-hexen-1-ol,(E)-3-hexen-1-ol和(E)-4-hexen-1-ol 1.01×10〜5 Pa。相应的速率常数为8.53±1.36、10.1±1.6、7.86±1.30、8.08±1.33、9.10±1.50和7.14±1.20(以10〜(-11)cm〜3分子为单位)使用相对技术分别通过火焰离子化检测器(GC-FID)通过气相色谱法测量〜(-1)s〜(-1))。还对这些反应进行了有关加成OH和H的反应通道的理论计算,以进一步了解反应机理和H吸收反应的相对重要性。与先前报道的结果相反,H吸收通道是O​​H自由基与这些己烯醇反应的不可忽略的反应通道。 H吸收通道的速率常数与OH加成通道的速率常数相当,并且对大多数研究的醇贡献> 20%,对于(E)-3-hexen-1-ol甚至贡献> 50%。因此,H吸收通道可能在这些醇与OH自由基的反应中起重要作用,必须在某些大气化学机理和模型中加以考虑。

著录项

  • 来源
    《Environmental Science & Technology》 |2015年第17期|10380-10388|共9页
  • 作者单位

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China;

    Key Laboratory of Atmospheric Composition and Optical Radiation, Anhui Institute of Optics and Fine Mechanics Chinese Academy of Sciences, Hefei 230031, Anhui, China,Laboratory of Atmospheric Physico-Chemistry, Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, Anhui, China,School of Environmental Science and Optoelectronic Technology, University of Science and Technology of China, Hefei 230026, Anhui, China;

    College of Information Engineering, Guizhou Minzu University, Guiyang 550025, China;

    Department of Physics, Guizhou University, Guiyang 550025, China;

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  • 正文语种 eng
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  • 入库时间 2022-08-17 13:59:45

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