Kelly Patricia D, Bright Cameron C, Blanksby Stephen J, da Silva Gabriel, Trevitt Adam J
School of Chemistry and Molecular Bioscience , University of Wollongong , Wollongong 2522 , Australia.
Central Analytical Research Facility, Institute for Future Environments , Queensland University of Technology , Brisbane 4001 , Australia.
J Phys Chem A. 2019 Oct 17;123(41):8881-8892. doi: 10.1021/acs.jpca.9b04088. Epub 2019 Oct 2.
Protonated aniline-one of the simplest nitrogen-bearing aromatic molecules-is speculated to be present within Titan's atmosphere, where it could play a role in molecular weight growth chemistry. To investigate this possibility, this paper examines the reactions of propene with distonic radical cations derived from protonated aniline. The reaction kinetics, products, and branching ratios of these distonic radical cations (i.e., 2-, 3-, and 4-dehydroanilinium radical cations) are measured in the gas phase using ion-trap mass spectrometry, and calculations (M06-2/6-31G(2df,p) and G3X-K) are used to rationalize the results. The reaction efficiencies for the 2-, 3-, and 4-dehydroanilinium radical cations are reported as 30.7 (±3.1)%, 2.4 (±0.5)%, and 2.1 (±0.4)%, respectively (with ±50% absolute accuracy). The 4- and 3-dehydroanilinium radical cations undergo addition of propene followed by either (i) methyl radical loss forming ammonio styrene cations (/ 120) or (ii) ethylene loss pathways forming the ammonio benzyl radical cation (/ 107). The 4-dehydroanilinium reaction favors methyl loss over ethylene loss, whereas the reverse is true for 3-dehydroanilinium. In contrast, the 2-dehydroanilinium radical cation reacts with propene to purportedly form amino tropylium cation (/ 106) with ethyl radical loss and methyl amino tropylium cation (/ 120) with methyl radical loss. The energies of all minima and transition states leading to predicted dissociation products are below the energy of the initial reactants providing plausible pathways at the low temperatures of Titan's atmosphere.
质子化苯胺是最简单的含氮芳香分子之一,据推测存在于土卫六的大气层中,在那里它可能在分子量增长化学过程中发挥作用。为了研究这种可能性,本文研究了丙烯与质子化苯胺衍生的双自由基阳离子的反应。使用离子阱质谱法在气相中测量了这些双自由基阳离子(即2-、3-和4-脱氢苯胺阳离子)的反应动力学、产物和分支比,并使用计算方法(M06-2/6-31G(2df,p) 和G3X-K)来解释结果。2-、3-和4-脱氢苯胺阳离子的反应效率分别报告为30.7 (±3.1)%、2.4 (±0.5)% 和2.1 (±0.4)%(绝对准确度为±50%)。4-和3-脱氢苯胺阳离子先与丙烯加成,然后要么(i)失去甲基形成铵基苯乙烯阳离子(/ 120),要么(ii)失去乙烯形成铵基苄基自由基阳离子(/ 107)。4-脱氢苯胺反应中甲基损失比乙烯损失更有利,而3-脱氢苯胺则相反。相比之下,2-脱氢苯胺阳离子与丙烯反应据称形成失去乙基的氨基环庚三烯阳离子(/ 106)和失去甲基的甲基氨基环庚三烯阳离子(/ 120)。导致预测解离产物的所有极小值和过渡态的能量都低于初始反应物的能量,这为土卫六大气层低温下的反应提供了合理的途径。