H2 formation on PAHs in photodissociation regions: a high-temperature pathway to molecular hydrogen
Leon Boschman, St\'ephanie Cazaux, Marco Spaans, Ronnie Hoekstra,, Thomas Schlath\"olter

TL;DR
This study models how polycyclic aromatic hydrocarbons (PAHs) contribute to molecular hydrogen formation in photodissociation regions, especially at high temperatures, significantly affecting cloud structure and H2 formation rates.
Contribution
It introduces a high-temperature H2 formation pathway on PAHs and demonstrates its impact on PDR modeling and cloud structure, expanding understanding beyond dust grain chemistry.
Findings
H2 formation on PAHs is efficient at T > 200 K.
PAHs influence the atomic-to-molecular hydrogen transition depth.
H2 formation rates on PAHs can match observed high rates in PDRs.
Abstract
Molecular hydrogen is the most abundant molecule in the Universe. It is thought that a large portion of H2 forms by association of hydrogen atoms to polycyclic aromatic hydrocarbons (PAHs). We model the influence of PAHs on total H2 formation rates in photodissociation regions (PDRs) and assess the effect of these formation rates on the total cloud structure. We set up a chemical kinetic model at steady state in a PDR environment and included adiative transfer to calculate the chemistry at different depths in the PDR. This model includes known dust grain chemistry for the formation of H2 and a H2 formation mechanism on PAHs. Since H2 formation on PAHs is impeded by thermal barriers, this pathway is only efficient at higher temperatures (T > 200 K). At these temperatures the conventional route of H2 formation via H atoms physisorbed on dust grains is no longer feasible, so the PAH…
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