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首页> 外文期刊>The Journal of Chemical Physics >Nascent energy distribution of the Criegee intermediate CH2OO from direct dynamics calculations of primary ozonide dissociation
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Nascent energy distribution of the Criegee intermediate CH2OO from direct dynamics calculations of primary ozonide dissociation

机译:从初级臭氧解离直接动力学计算的Criegee中间CH2OO的新生能量分布

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摘要

Ozonolysis produces chemically activated carbonyl oxides (Criegee intermediates, CIs) that are either stabilized or decompose directly. This branching has an important impact on atmospheric chemistry. Prior theoretical studies have employed statistical models for energy partitioning to the CI arising from dissociation of the initially formed primary ozonide (POZ). Here, we used direct dynamics simulations to explore this partitioning for decomposition of c-C2H4O3, the POZ in ethylene ozonolysis. A priori estimates for the overall stabilization probability were then obtained by coupling the direct dynamics results with master equation simulations. Trajectories were initiated at the concerted cycloreversion transition state, as well as the second transition state of a stepwise dissociation pathway, both leading to a CI (H2COO) and formaldehyde (H2CO). The resulting CI energy distributions were incorporated in master equation simulations of CI decomposition to obtain channel-specific stabilized CI (sCI) yields. Master equation simulations of POZ formation and decomposition, based on newhigh-level electronic structure calculations, were used to predict yields for the different POZ decomposition channels. A non-negligible contribution of stepwise POZ dissociation was found, and new mechanistic aspects of this pathway were elucidated. By combining the trajectory-based channel-specific sCI yields with the channel branching fractions, an overall sCI yield of (48 +/- 5)% was obtained. Non-statistical energy release was shown to measurably affect sCI formation, with statistical models predicting significantly lower overall sCI yields (similar to 30%). Within the range of experimental literature values (35%-54%), our trajectory-based calculations favor those clustered at the upper end of the spectrum. Published by AIP Publishing.
机译:臭氧分解产生稳定或分解的化学活性羰基氧化物(Criaegee中间体,顺式)。该分支对大气化学产生了重要影响。现有的理论研究已经采用统计模型用于从初始形成的原发性臭氧(POZ)的解离引起的CI的能量分配。在这里,我们使用直接动态模拟来探讨C-C2H4O3分解的这种分区,乙烯臭氧中的POZ。然后通过将直接动力学结果与主方程模拟耦合来获得整体稳定概率的先验估计。在齐齐齐全的环肠过渡状态下启动轨迹,以及阶梯式解离途径的第二转变状态,导致C 1(H2COO)和甲醛(H2CO)。将得到的CI能量分布纳入CI分解的母体方程模拟中,以获得特异性稳定的Ci(SCI)产量。基于Newhigh级电子结构计算的POZ形成和分解的主方程模拟用于预测不同POZ分解通道的产量。发现了逐步Poz解离的不可忽略的贡献,并阐明了该途径的新机制方面。通过将基于轨迹的频道特异性SCI产生与通道支化分数相结合,得到了(48 +/- 5)%的总体SCI产率。显示非统计能量释放可测量地影响SCI形成,统计模型预测总体SCI产量显着降低(类似于30%)。在实验文献值范围内(35%-54%),我们的轨迹基计算有利于在光谱的上端聚集的计算。通过AIP发布发布。

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