Understanding how to catalytically break the C–H
bond of
aromatic molecules, such as polycyclic aromatic hydrocarbons (PAHs),
is currently a big challenge and a subject of study in catalysis,
astrochemistry, and planetary science. In the latter, the study of
the breakdown reaction of PAHs on mineral surfaces is important to
understand if PAHs are linked to prebiotic molecules in regions of
star and planet formation. In this work, we employed a periodic density
functional theory along with Grimme’s D4 (DFT-D4) approach
for studying the adsorption of a sample of PAHs (naphthalene, anthracene,
fluoranthene, pyrene, coronene, and benzocoronene) and fullerene on
the [010] forsterite surface and its defective surfaces (Fe-doped
and Ni-doped surfaces and a MgO-Schottky vacancy) for their implications
in catalysis and astrochemistry. On the basis of structural and binding
energy analysis, large PAHs and fullerene present stronger adsorption
on the pristine, Fe-doped, and Ni-doped forsterite surfaces than small
PAHs. On a MgO-Schottky vacancy, parallel adsorption of the PAH leads
to the chemisorption process (C–Si and/or C–O bonds),
whereas perpendicular orientation of the PAH leads to the catalytic
breaking of the aromatic C–H bond via a barrierless reaction.
Spin density and charge analysis show that C–H dissociation
is promoted by electron donation from the vacancy to the PAH. As a
result of the undercoordinated Si and O atoms, the vacancy acts as
a Frustrated Lewis Pair (FLP) catalyst. Therefore, a MgO-Schottky
vacancy [010] forsterite surface proved to have potential catalytic
activity for the activation of C–H bond in aromatic molecules.