Abstract
We have investigated the response of superhydrogenated gas-phase
coronene cations upon soft x-ray absorption. Carbon
(1s)⟶π⋆ transitions were resonantly excited at
hν =285 eV. The resulting core hole is then filled in an Auger decay
process, with the excess energy being released in the form of an Auger
electron. Predominantly highly excited dications are thus formed, which
cool down by hydrogen emission. In superhydrogenated systems, the
additional H atoms act as a buffer, quenching loss of native H atoms and
molecular fragmentation. Dissociation and transition state energies for
several H loss channels were computed by means of density functional
theory. Using these energies as input into an Arrhenius-type cascade
model, very good agreement with the experimental data is found. The
results have important implications for the survival of polyaromatic
hydrocarbons in the interstellar medium and reflect key aspects of
graphene hydrogenation.
| Original language | English |
|---|---|
| Article number | 053002 |
| Journal | Physical Review Letters |
| Volume | 113 |
| DOIs | |
| Publication status | Published - Aug-2014 |
Keywords
- Inner-shell excitation and ionization
- Photon interactions with molecules
- Molecular and chemical processes and interactions
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