A detailed understanding
of the water–semiconductor interface
is of major importance for elucidating the molecular interactions
at the photocatalyst’s surface. Here, we studied the effect
of vacancy defects on the adsorption of a water molecule on the (101̅0)
and (112̅0) CdS surfaces, using spin-polarized density functional
theory. We observed that the local spin polarization did not persist
for most of the cationic vacancies on the surfaces, unlike in bulk,
owing to surface reconstructions caused by displaced S atoms. This
result suggests that cationic vacancies on these surfaces may not
be the leading cause of the experimentally observed magnetism in CdS
nanostructures. The surface vacancies are predominantly nonmagnetic
except for one case, where a magnetic cationic vacancy is relatively
stable due to constraints posed by the (101̅0) surface geometry.
At this particular magnetic defect site, we found a very strong interaction
with the H2O molecule leading to a case of chemisorption,
where the local spin polarization vanishes concurrently. At the same
defect site, adsorption of an O2 molecule was also simulated,
and the results were found to be consistent with experimental electron
paramagnetic resonance findings for powdered CdS. The anion vacancies
on these surfaces were always found to be nonmagnetic and did not
affect the water adsorption at these surfaces.