PAH chemistry at eV internal energies. 1. H-shifted isomers
Georges Trinquier, Aude Simon, Mathias Rapacioli, Florent Xavier, Gad\'ea

TL;DR
This study investigates hydrogen-shifted isomers of PAHs at high internal energies using DFT calculations, revealing their energetic properties and potential relevance in astrophysical environments.
Contribution
It provides detailed computational analysis of H-shifted PAH isomers, highlighting their energetic landscape and differences between neutral and cationic states, which was previously underexplored.
Findings
H-shifted isomers are 4-5 eV above regular forms
Barriers to isomerization are about 1 eV
Cationic PAHs have lower energy H-shifted minima
Abstract
The PAH family of organic compounds (polycyclic aromatic hydrocarbons), involved in several fields of chemistry, has received particular attention in astrochemistry, where their vibrational spectroscopy, thermodynamic, dynamic, and fragmentation properties are now abundantly documented. This survey aims at drawing trends for low spin-multiplicity surfaces of PAHs bearing internal energies in the range 1-10 eV. It addresses some typical alternatives to the ground-state regular structures of PAHs, making explicit possible intramolecular rearrangements leading to high-lying minima. These isomerisations should be taken into consideration when addressing PAH processing in astrophysical conditions. The first part of this double-entry study focuses on the hydrogen-shifted forms, which bear both a carbene center and a saturated carbon. It rests upon DFT calculations mainly performed on two…
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