Department of Physics, Federal University of Amazonas, Manaus 69067-005, Amazonas, Brazil.
J Phys Chem A. 2023 Apr 27;127(16):3551-3559. doi: 10.1021/acs.jpca.2c08572. Epub 2023 Apr 17.
Malic acid (MA) (CHO) is one of the most important organic constituents of fruits that is widely used in food and beverage industries. It is also detected in the atmospheric aerosol samples collected in different parts of the world. Considering the fact that secondary organic aerosols have adverse impacts on the global atmosphere and climate and a molecular-level understanding of the compositions and formation mechanism of secondary organic aerosols is necessary, we have performed systematic density functional electronic structure calculations to investigate the hydrogen-bonding interactions between MA and several naturally occurring nitrogen-containing atmospheric bases such as ammonia and amines that are derived from ammonia by the substitution of hydrogens by a methyl group. The base molecules were allowed to interact with the carboxylic COOH and the hydroxyl-OH group of the MA separately. While at both sites, MA produces energetically stable binary complexes with bases with large negative values of binding energy, the thermodynamical stability, at an ambient temperature and pressure of 298.15 K and 1 atm, respectively, is favored only for the clusters formed at the COOH site. A much larger red shift of the carboxylic-OH stretch than that of the hydroxyl-OH reinforces the preference of this site for cluster formation. Both the binding electronic energy and binding free energy of MA-ammonia complexes are lower than those of MA-amine complexes, although the amines are derivatives of NH. The large increase in the Rayleigh activities upon cluster formation indicates that the MA-atmospheric base cluster may interact strongly with solar radiation. The detailed analysis of the structural, energetic, electrical, and spectroscopic properties of the binary complexes formed by MA with atmospheric bases shows that MA could participate in the atmospheric nucleation processes and subsequently contribute effectively to new particle formation in the atmosphere.
苹果酸(MA)(CHO)是水果中最重要的有机成分之一,广泛应用于食品和饮料行业。它也在世界不同地区采集的大气气溶胶样本中被检测到。考虑到二次有机气溶胶对全球大气和气候有不利影响,需要对其组成和形成机制进行分子水平的了解,我们进行了系统的密度泛函电子结构计算,以研究 MA 与几种天然存在的含氮大气碱基之间的氢键相互作用,如氨和由氨取代氢得到的甲基取代的胺。允许碱基分子分别与 MA 的羧酸 COOH 和羟基-OH 基团相互作用。虽然在这两个位置,MA 都与碱基形成了具有大负值结合能的稳定二元配合物,但在环境温度和压力分别为 298.15 K 和 1 atm 的热力学稳定性仅有利于在 COOH 位置形成的簇。羧酸-OH 伸缩的红移比羟基-OH 大得多,这增强了该位置对簇形成的偏好。MA-氨配合物的结合电子能和结合自由能都低于 MA-胺配合物,尽管胺是 NH 的衍生物。簇形成后 Rayleigh 活性的大幅增加表明 MA-大气碱基簇可能与太阳辐射强烈相互作用。对 MA 与大气碱基形成的二元配合物的结构、能量、电学和光谱性质的详细分析表明,MA 可以参与大气成核过程,并随后有效地促进大气中新粒子的形成。