Formation of acetonitrile (CH3CN) under cold interstellar, tropospheric and combustion mediums

The knowledge of the formation of gas-phase carcinogenic acetonitrile (CH<sub>3</sub>CN) is limited in interstellar, troposphere, and combustion mediums; thus, its formation and fate are of great importance for all these gas-phase environments when accessing its toxicity and its wide range of applications. In this work, we propose a mechanism for the formation of CH<sub>3</sub>CN from the reaction of OH/O<sub>2</sub> on ethanimine (CH<sub>3</sub>CH=NH) using ab initio/Density Functional Theory (DFT) potential energy surface in combination with microcanonical variational transition state theory (µVTST) and Ramsperger-Kassel-Marcus (RRKM)/master equation (ME) simulation to predict the rate constants and branching fraction in the temperature range of 100 K to 1000 K and pressure range of 0.0001 bar to 100 bar. The reaction starts with cis (Z) and trans (E) CH<sub>3</sub>CH=NH isomer with OH radical followed by spontaneous formation via pre-reactive complex, forming the carbon and nitrogen-centered radicals. The O<sub>2</sub> radical then attacks the carbon and nitrogen-centered radicals to form acetonitrile (CH<sub>3</sub>CN) and HO<sub>2</sub> radicals. The results show that N-H and C-H dominate the H-atoms abstraction by OH radicals is similar to its isoelectronic analogous reaction system, i.e., CH<sub>3</sub>CHO + OH/O<sub>2</sub> and CH<sub>3</sub>CHCH<sub>2</sub> + OH/O<sub>2</sub> and similar to methanimine (CH<sub>2</sub>NH) systems. The calculated rate constants for OH-initiated oxidation of CH<sub>3</sub>CH=NH are in the range of ~ 10<sup>-11</sup> cm<sup>3</sup> molecule<sup>-1</sup> s<sup>-1</sup> (at 300 K) and are in very good agreement with previous experimental values of its isoelectronic reaction system. The atmospheric lifetime due to the loss of CH<sub>3</sub>CHNH by OH radical (10 to 11 h) is in very good agreement with the similar pollutants in the troposphere temperature range between 200 and 320 K. The results indicate that its contribution to global warming is negligible. However, the formation of products such as CH<sub>3</sub>CN may interact with other atmospheric species, which could lead to the production of potentially hazardous compounds such as cyanogen (N<sub>2</sub>C<sub>2</sub>) and hydrogen cyanide (HCN).

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Publication Details

Journal
Scientific Reports
Published
2024-09-27
DOI
https://doi.org/10.1038/s41598-024-70721-y
Citations
2
Primary Topic
Molecular Spectroscopy and Structure
Type
article
Field-Weighted Citation Impact
0.48

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article

Formation of acetonitrile (CH3CN) under cold interstellar, tropospheric and combustion mediums

R Saswathy, Mohamad Akbar Ali
2 citations
Scientific Reports
Molecular Spectroscopy and Structure
0.48
article

Formation of acetonitrile (CH3CN) under cold interstellar, tropospheric and combustion mediums

R Saswathy, Mohamad Akbar Ali
article en
2 citations

Abstract

The knowledge of the formation of gas-phase carcinogenic acetonitrile (CH<sub>3</sub>CN) is limited in interstellar, troposphere, and combustion mediums; thus, its formation and fate are of great importance for all these gas-phase environments when accessing its toxicity and its wide range of applications. In this work, we propose a mechanism for the formation of CH<sub>3</sub>CN from the reaction of OH/O<sub>2</sub> on ethanimine (CH<sub>3</sub>CH=NH) using ab initio/Density Functional Theory (DFT) potential energy surface in combination with microcanonical variational transition state theory (µVTST) and Ramsperger-Kassel-Marcus (RRKM)/master equation (ME) simulation to predict the rate constants and branching fraction in the temperature range of 100 K to 1000 K and pressure range of 0.0001 bar to 100 bar. The reaction starts with cis (Z) and trans (E) CH<sub>3</sub>CH=NH isomer with OH radical followed by spontaneous formation via pre-reactive complex, forming the carbon and nitrogen-centered radicals. The O<sub>2</sub> radical then attacks the carbon and nitrogen-centered radicals to form acetonitrile (CH<sub>3</sub>CN) and HO<sub>2</sub> radicals. The results show that N-H and C-H dominate the H-atoms abstraction by OH radicals is similar to its isoelectronic analogous reaction system, i.e., CH<sub>3</sub>CHO + OH/O<sub>2</sub> and CH<sub>3</sub>CHCH<sub>2</sub> + OH/O<sub>2</sub> and similar to methanimine (CH<sub>2</sub>NH) systems. The calculated rate constants for OH-initiated oxidation of CH<sub>3</sub>CH=NH are in the range of ~ 10<sup>-11</sup> cm<sup>3</sup> molecule<sup>-1</sup> s<sup>-1</sup> (at 300 K) and are in very good agreement with previous experimental values of its isoelectronic reaction system. The atmospheric lifetime due to the loss of CH<sub>3</sub>CHNH by OH radical (10 to 11 h) is in very good agreement with the similar pollutants in the troposphere temperature range between 200 and 320 K. The results indicate that its contribution to global warming is negligible. However, the formation of products such as CH<sub>3</sub>CN may interact with other atmospheric species, which could lead to the production of potentially hazardous compounds such as cyanogen (N<sub>2</sub>C<sub>2</sub>) and hydrogen cyanide (HCN).

Scientific ReportsVol. 14(1)
Khalifa University of Science and Technology (AE)
Khalifa University of Science, Technology and Research
Openalex Percentile: Top 40%
Molecular Spectroscopy and Structure
0.48
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