Abstract
We present experimental data on H2 formation processes on gas-phase polycyclic aromatic hydrocarbon (PAH) cations. This process was studied by exposing coronene radical cations, confined in a radio-frequency ion trap, to gas-phase H atoms. Sequential attachment of up to 23 hydrogen atoms has been observed. Exposure to atomic D instead of H allows one to distinguish attachment from competing abstraction reactions, as the latter now leave a unique fingerprint in the measured mass spectra. Modelling of the experimental results using realistic cross-sections and barriers for attachment and abstraction yield a 1:2 ratio of abstraction to attachment cross-sections. The strong contribution of abstraction indicates that H2 formation on interstellar PAH cations is an order of magnitude more relevant than previously thought.
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Foley, N., Cazaux, S., Egorov, D., Boschman, L. M. P. V., Hoekstra, R., & Schlathölter, T. (2018). Molecular hydrogen formation on interstellar PAHs through Eley-Rideal abstraction reactions. Monthly Notices of the Royal Astronomical Society, 479(1), 649–656. https://doi.org/10.1093/mnras/sty1528
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