TY - JOUR
T1 - Deexcitation Dynamics of Superhydrogenated Polycyclic Aromatic Hydrocarbon Cations after Soft-x-Ray Absorption
AU - Reitsma, Geert
AU - Boschman, Leon
AU - Deuzeman, Mart Johan
AU - Gonzalez Magana, Olmo
AU - Hoekstra, Steven
AU - Cazaux, Stéphanie
AU - Hoekstra, Ronnie
AU - Schlathölter, Thomas
PY - 2014/8
Y1 - 2014/8
N2 - 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.
AB - 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.
KW - Inner-shell excitation and ionization
KW - Photon interactions with molecules
KW - Molecular and chemical processes and interactions
UR - http://adsabs.harvard.edu/abs/2014PhRvL.113e3002R
U2 - 10.1103/PhysRevLett.113.053002
DO - 10.1103/PhysRevLett.113.053002
M3 - Article
SN - 0031-9007
VL - 113
JO - Physical Review Letters
JF - Physical Review Letters
M1 - 053002
ER -