Suppr超能文献

在寒冷的星际、对流层和燃烧介质中乙腈(CHCN)的形成。

Formation of acetonitrile (CHCN) under cold interstellar, tropospheric and combustion mediums.

作者信息

Ali Mohamad Akbar, R Saswathy

机构信息

Department of Chemistry, Khalifa University of Science and Technology, P.O. Box 127788, Abu Dhabi, UAE.

Center for the Catalyst and Separations, Khalifa University of Science and Technology, P.O. Box 127788, Abu Dhabi, UAE.

出版信息

Sci Rep. 2024 Sep 27;14(1):22313. doi: 10.1038/s41598-024-70721-y.

Abstract

The knowledge of the formation of gas-phase carcinogenic acetonitrile (CHCN) is limited in interstellar, troposphere, and combustion mediums; thus, its formation and fate are of great importance for all these gas-phase environments when accessing its toxicity and its wide range of applications. In this work, we propose a mechanism for the formation of CHCN from the reaction of OH/O on ethanimine (CHCH=NH) using ab initio/Density Functional Theory (DFT) potential energy surface in combination with microcanonical variational transition state theory (µVTST) and Ramsperger-Kassel-Marcus (RRKM)/master equation (ME) simulation to predict the rate constants and branching fraction in the temperature range of 100 K to 1000 K and pressure range of 0.0001 bar to 100 bar. The reaction starts with cis (Z) and trans (E) CHCH=NH isomer with OH radical followed by spontaneous formation via pre-reactive complex, forming the carbon and nitrogen-centered radicals. The O radical then attacks the carbon and nitrogen-centered radicals to form acetonitrile (CHCN) and HO radicals. The results show that N-H and C-H dominate the H-atoms abstraction by OH radicals is similar to its isoelectronic analogous reaction system, i.e., CHCHO + OH/O and CHCHCH + OH/O and similar to methanimine (CHNH) systems. The calculated rate constants for OH-initiated oxidation of CHCH=NH are in the range of ~ 10 cm molecule s (at 300 K) and are in very good agreement with previous experimental values of its isoelectronic reaction system. The atmospheric lifetime due to the loss of CHCHNH by OH radical (10 to 11 h) is in very good agreement with the similar pollutants in the troposphere temperature range between 200 and 320 K. The results indicate that its contribution to global warming is negligible. However, the formation of products such as CHCN may interact with other atmospheric species, which could lead to the production of potentially hazardous compounds such as cyanogen (NC) and hydrogen cyanide (HCN).

摘要

在星际、对流层和燃烧介质中,气相致癌物质乙腈(CH₃CN)的形成机制尚不明确;因此,在评估其毒性及其广泛应用时,乙腈的形成和归宿对于所有这些气相环境而言都至关重要。在这项工作中,我们利用从头算/密度泛函理论(DFT)势能面,结合微正则变分过渡态理论(µVTST)和拉姆施佩格-卡塞尔-马库斯(RRKM)/主方程(ME)模拟,提出了一种由乙亚胺(CH₃CH=NH)与OH/O反应生成CH₃CN的机制,以预测100 K至1000 K温度范围和0.0001 bar至100 bar压力范围内的速率常数和分支比。该反应始于顺式(Z)和反式(E)CH₃CH=NH异构体与OH自由基,随后通过预反应复合物自发形成,生成以碳和氮为中心的自由基。然后,O自由基攻击以碳和氮为中心的自由基,形成乙腈(CH₃CN)和HO自由基。结果表明,N-H和C-H主导了OH自由基夺取H原子的过程,这与其等电子类似反应体系,即CH₃CHO + OH/O和CH₃CH=CH₂ + OH/O相似,也与甲亚胺(CH₂NH)体系相似。计算得出的OH引发的CH₃CH=NH氧化反应的速率常数在~10⁻¹³ cm³ molecule⁻¹ s⁻¹范围内(在300 K时),与此前等电子反应体系的实验值非常吻合。在200至320 K的对流层温度范围内,由于OH自由基导致CH₃CHNH损失的大气寿命为10至11小时,与类似污染物的情况非常吻合。结果表明,其对全球变暖的贡献可忽略不计。然而,CH₃CN等产物的形成可能会与其他大气物种相互作用,这可能导致生成潜在危险化合物,如氰(NC)和氰化氢(HCN)。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7ec1/11436810/cf684c498e95/41598_2024_70721_Fig1_HTML.jpg

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验