Stereodynamics of the Charge Transfer Reactions between N <sub>2</sub> <sup>+</sup> and O <sub>2</sub>

In this work, we investigate ion-molecule reactions N<sub>2</sub><sup>+</sup> + O<sub>2</sub> → N<sub>2</sub> + O<sub>2</sub><sup>+</sup>/N<sub>2</sub> + O<sup>+</sup> + O with the collision energies from 0.59 to 4.92 eV using the crossed-beam velocity map imaging technique, given the essential roles in atmospheric chemistry. For the charge exchange (CE) reactions at higher collision energies, the long-range collision leads to the forward-scattered O<sub>2</sub><sup>+</sup> ions, while the O<sub>2</sub><sup>+</sup> ions produced at the lowest collision energy of 0.59 eV show a diffuse distribution but basically along the collision axis. The latter is attributed to the formation of the long-lived intermediate complex [N<sub>2</sub>O<sub>2</sub>]<sup>+</sup>** in a short-range collision. Diffuse distributions of the O<sup>+</sup> yield of dissociative charge exchange (DCE) are observed at 3.93 and 4.92 eV. By the data analyses using the Doppler kinematics model, we find that these O<sup>+</sup> ions are produced not only from the predissociative O<sub>2</sub><sup>+</sup>** but also the intermediate N<sub>2</sub>O<sup>+</sup>**, and these two intermediates can be formed, respectively, by the long-range and initimate collisions. The branching ratios of different DCE pathways are estimated, indicating the predominance of the N<sub>2</sub>O<sup>+</sup>**-experienced pathways at relatively high collision energy.

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Publication Details

Journal
The Journal of Physical Chemistry A
Published
2025-11-27
DOI
https://doi.org/10.1021/acs.jpca.5c05080
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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article

Stereodynamics of the Charge Transfer Reactions between N 2 + and O 2

Qiang Guo, Jie Hu, Shan Xi Tian, Yaya Zhi
The Journal of Physical Chemistry A
Astrophysics and Star Formation Studies
article

Stereodynamics of the Charge Transfer Reactions between N 2 + and O 2

Qiang Guo, Jie Hu, Shan Xi Tian, Yaya Zhi
article en

Abstract

In this work, we investigate ion-molecule reactions N<sub>2</sub><sup>+</sup> + O<sub>2</sub> → N<sub>2</sub> + O<sub>2</sub><sup>+</sup>/N<sub>2</sub> + O<sup>+</sup> + O with the collision energies from 0.59 to 4.92 eV using the crossed-beam velocity map imaging technique, given the essential roles in atmospheric chemistry. For the charge exchange (CE) reactions at higher collision energies, the long-range collision leads to the forward-scattered O<sub>2</sub><sup>+</sup> ions, while the O<sub>2</sub><sup>+</sup> ions produced at the lowest collision energy of 0.59 eV show a diffuse distribution but basically along the collision axis. The latter is attributed to the formation of the long-lived intermediate complex [N<sub>2</sub>O<sub>2</sub>]<sup>+</sup>** in a short-range collision. Diffuse distributions of the O<sup>+</sup> yield of dissociative charge exchange (DCE) are observed at 3.93 and 4.92 eV. By the data analyses using the Doppler kinematics model, we find that these O<sup>+</sup> ions are produced not only from the predissociative O<sub>2</sub><sup>+</sup>** but also the intermediate N<sub>2</sub>O<sup>+</sup>**, and these two intermediates can be formed, respectively, by the long-range and initimate collisions. The branching ratios of different DCE pathways are estimated, indicating the predominance of the N<sub>2</sub>O<sup>+</sup>**-experienced pathways at relatively high collision energy.

The Journal of Physical Chemistry AVol. 130(4)
University of Science and Technology of China (CN), Dalian Institute of Chemical Physics (CN), Chinese Academy of Sciences (CN), Hefei National Center for Physical Sciences at Nanoscale (CN), Microscale (United States) (US)
Openalex Percentile: Top 74%
Astrophysics and Star Formation Studies
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