Long Bo, Xia Yu, Truhlar Donald G
College of Materials Science and Engineering, Guizhou Minzu University, Guiyang550025, China.
Department of Chemistry, Chemical Theory Center, and Minnesota Supercomputing Institute, University of Minnesota, Minneapolis, Minnesota55455-0431, United States.
J Am Chem Soc. 2022 Nov 2;144(43):19910-19920. doi: 10.1021/jacs.2c07994. Epub 2022 Oct 20.
Kinetics provides the fundamental parameters for elucidating sources and sinks of key atmospheric species and for atmospheric modeling more generally. Obtaining quantitative kinetics in the laboratory for the full range of atmospheric temperatures and pressures is quite difficult. Here, we use computational chemistry to obtain quantitative rate constants for the reactions of HO with HCHO, CHCHO, and CFCHO. First, we calculate the high-pressure-limit rate constants by using a dual-level strategy that combines conventional transition state theory using a high level of electronic structure wave function theory with canonical variational transition state theory including small-curvature tunneling using density functional theory. The wave-function level is beyond-CCSD(T) for HCHO and CCSD(T)-F12a (Level-A) for XCHO (X = CH, CF), and the density functional (Level-B) is specifically validated for these reactions. Then, we calculate the pressure-dependent rate constants by using system-specific quantum RRK theory (SS-QRRK) and also by an energy-grained master equation. The two treatments of the pressure dependence agree well. We find that the Level-A//Level-B method gives good agreement with CCSDTQ(P)/CBS. We also find that anharmonicity is an important factor that increases the rate constants of all three reactions. We find that the HO + HCHO reaction has a significant dependence on pressure, but the HO + CFCHO reaction is almost independent of pressure. Our findings show that the HO + HCHO reaction makes important contribution to the sink for HCHO, and the HO + CFCHO reaction is the dominant sink for CFCHO in the atmosphere.
动力学为阐明关键大气物种的源和汇以及更广泛的大气建模提供了基本参数。在实验室中获取涵盖所有大气温度和压力范围的定量动力学数据相当困难。在此,我们使用计算化学来获取HO与HCHO、CHCHO和CFCHO反应的定量速率常数。首先,我们采用一种双水平策略计算高压极限速率常数,该策略将使用高水平电子结构波函数理论的传统过渡态理论与包含使用密度泛函理论的小曲率隧道效应的正则变分过渡态理论相结合。对于HCHO,波函数水平为超越耦合簇单双激发组态相互作用并包括微扰三重激发(CCSD(T));对于XCHO(X = CH、CF),波函数水平为CCSD(T)-F12a(A水平),并且密度泛函(B水平)已针对这些反应进行了专门验证。然后,我们使用特定系统的量子 Rice-Ramsperger-Kassel 理论(SS-QRRK)以及能量粒度主方程来计算压力依赖的速率常数。对压力依赖性的两种处理方法结果吻合良好。我们发现A水平//B水平方法与完全耦合簇单双激发组态相互作用并包括微扰四重激发及完全基组外推(CCSDTQ(P)/CBS)结果吻合良好。我们还发现非谐性是增加所有三个反应速率常数的一个重要因素。我们发现HO + HCHO反应对压力有显著依赖性,但HO + CFCHO反应几乎与压力无关。我们的研究结果表明,HO + HCHO反应对HCHO的汇有重要贡献,并且HO + CFCHO反应是大气中CFCHO的主要汇。