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电子诱导甲醇-一氧化碳冰处理过程中甲酸甲酯生成的机理。

Mechanisms of methyl formate production during electron-induced processing of methanol-carbon monoxide ices.

机构信息

Universität Bremen, Fachbereich 2 (Chemie/Biologie), Institut für Angewandte und Physikalische Chemie, Leobener Straße 5, D-28359 Bremen, Germany.

出版信息

Phys Chem Chem Phys. 2021 May 26;23(20):11649-11662. doi: 10.1039/d1cp01255j.

DOI:10.1039/d1cp01255j
PMID:33978008
Abstract

The formation of methyl formate (CH3OCHO) upon electron irradiation of mixed ices of carbon monoxide (CO) and methanol (CH3OH) has been monitored by post-irradiation thermal desorption spectrometry (TDS). The energy dependence of the product yields obtained with electron energies between 3 and 18 eV was studied. These energies are characteristic of secondary electrons that are released in vast numbers under the effect of ionizing radiation. Our results reveal that the reactions leading to methyl formate are initiated by a number of different electron-molecule interactions that produce CH3O˙ radicals. Dissociative electron attachment (DEA) to CH3OH around 5.5 eV and neutral dissociation (ND) above 7 eV release CH3O˙ radicals that can add to CO to initiate a reaction sequence leading to formation of methyl formate. Around 10 eV, DEA to CO yields an oxygen radical anion that reacts with CH3OH to also produce CH3O˙ radicals. Alternatively, CH3OH can also release H˙ radicals upon both DEA and ND. These can also add to CO to form HCO˙ radicals as an intermediate to formaldehyde (H2CO), which was also investigated to unravel the reaction mechanisms leading to formation of methyl formate. The recombination of HCO˙ and CH3O˙ as minority radical species is considered as an alternative but less probable pathway to the formation of methyl formate. To the best of our knowledge, this is the first study showing considerable contributions of DEA to the formation of methyl formate in CH3OH containing ices. Thus, our study has important implications for current astrochemical models.

摘要

通过电子辐照一氧化碳 (CO) 和甲醇 (CH3OH) 混合冰的后辐照热解吸光谱法 (TDS) 监测到甲酸盐 (CH3OCHO) 的形成。研究了电子能量在 3 至 18 eV 之间时获得的产物产率的能量依赖性。这些能量是大量释放的二次电子的特征,这些二次电子是在电离辐射的作用下释放的。我们的结果表明,导致甲酸盐的反应是由许多不同的电子-分子相互作用引发的,这些相互作用产生了 CH3O˙自由基。在 5.5 eV 左右,甲醇的电子离解(DEA)和高于 7 eV 的中性解离(ND)释放 CH3O˙自由基,这些自由基可以与 CO 加成,引发导致甲酸盐形成的反应序列。在 10 eV 左右,DEA 到 CO 产生氧自由基阴离子,与 CH3OH 反应也产生 CH3O˙自由基。或者,CH3OH 也可以在 DEA 和 ND 时释放 H˙自由基。这些自由基也可以与 CO 加成形成 HCO˙自由基,作为甲醛 (H2CO) 的中间体,也研究了甲醛来揭示形成甲酸盐的反应机制。HCO˙和 CH3O˙作为少数自由基物种的复合被认为是形成甲酸盐的替代但不太可能的途径。据我们所知,这是首次研究表明 DEA 对甲醇冰中形成甲酸盐有相当大的贡献。因此,我们的研究对当前的天体化学模型具有重要意义。

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