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Substituent effects on H <sub/>3</sub><sup>+</sup> formation via H <sub/>2</sub> roaming mechanisms from organic molecules under strong-field photodissociation

DOI:10.1063/1.5065387 期刊:The Journal of Chemical Physics 出版年份:2018 更新时间:2025-09-23 15:23:52
摘要: Roaming chemical reactions are often associated with neutral molecules. The recent findings of roaming processes in ionic species, in particular, ones that lead to the formation of H3+ under strong-field laser excitation, are of considerable interest. Given that such gas-phase reactions are initiated by double ionization and subsequently facilitated through deprotonation, we investigate the strong-field photodissociation of ethanethiol, also known as ethyl mercaptan, and compare it to results from ethanol. Contrary to expectations, the H3+ yield was found to be an order of magnitude lower for ethanethiol at certain laser field intensities, despite its lower ionization energy and higher acidity compared to ethanol. In-depth analysis of the femtosecond time-resolved experimental findings, supported by ab initio quantum mechanical calculations, provides key information regarding the roaming mechanisms related to H3+ formation. Results of this study on the dynamics of dissociative half-collisions involving H3+, a vital cation which acts as a Br?nsted–Lowry acid protonating interstellar organic compounds, may also provide valuable information regarding the formation mechanisms and observed natural abundances of complex organic molecules in interstellar media and planetary atmospheres.
作者: Nagitha Ekanayake,Muath Nairat,Nicholas P. Weingartz,Matthew J. Michie,Benjamin G. Levine,Marcos Dantus
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To investigate the effect of functional group substitution (specifically, replacing hydroxyl with thiol group) on the yield and formation time scales of H3+ ions produced via H2 roaming mechanisms during strong-field photodissociation of organic molecules, using ethanethiol and ethanol as comparative cases.

The substitution of a thiol group for a hydroxyl group in organic molecules leads to a significant reduction in H3+ yield and an increase in formation time during strong-field photodissociation, due to less favorable electronic and structural changes upon double ionization. These findings provide insights into roaming mechanisms in ionic species and have implications for understanding chemical reactions in interstellar media.

The study is limited to gas-phase reactions under strong laser fields, which may not fully represent conditions in interstellar or atmospheric environments. The intensity calibration has an uncertainty factor of 2, and measurements are subject to noise in differential yield analysis. The computational methods rely on specific levels of theory (e.g., CCSD/aug-cc-pVDZ) which may not capture all electronic effects accurately.

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