posted on 2025-03-10, 06:09authored byFrederik G. Doktor, Niels M. Mikkelsen, Signe Kyrkjebo̷, Prashant Srivastava, Richard Balog, Bjo̷rk Hammer, Karina Morgenstern, Liv Hornekær
We
present a study on the initial stages of ice growth on pristine
and oxygen-functionalized highly oriented pyrolytic graphite (O-HOPG),
combining low-temperature scanning tunneling microscopy (LT-STM) and
machine-learning structural searches. LT-STM images show that oxygen
atoms act as nucleation sites for ice growth and that the size, structure,
and porosity of the nanometer-sized ice clusters depend strongly on
the growth temperature. Machine learning-assisted structural searches
and first-principles energy calculations confirm that clusters of
water molecules are likely to bind to chemisorbed oxygen atoms through
hydrogen bonding. During the early stages of the cluster growth, clusters
of water molecules are likely to be immobilized by binding to more
than one chemisorbed oxygen atom through hydrogen bonding. However,
the energy gain by hydrogen bond formation of a molecule, upon incorporation
into smaller clusters only bound to a single oxygen atom, is large
enough to induce cluster diffusion and favor the growth of larger
ice clusters. Our results demonstrate that the mobility of water molecules
is significantly lowered in the presence of defects on the surface.
The observed lower mobility on defected carbon presented here offers
an enhanced understanding of macroscopic anti-icing properties observed
for functionalized HOPG under ambient conditions and provides insight
into the early stages of ice growth on dust grain surfaces in interstellar
space.