In the present study,
alkaline earth metal scheelite-type ABO4 compounds (A =
Ca, Sr, and Ba; B = Mo and W) synthesized
by a hydrothermal method were systematically studied. The as-obtained
photocatalysts were characterized by X-ray diffraction (XRD), scanning
electron microscopy (SEM), Brunauer–Emmett–Teller (BET)
surface area analysis, UV–vis diffuse reflectance (DR/UV–vis)
spectroscopy, photoluminescence, and thermoluminescence (TL) spectroscopy
together with charge carrier lifetime measurements, electron paramagnetic
resonance (EPR) spectroscopy, and electrochemical impedance spectroscopy
(EIS). The photocatalytic activity was studied in the reaction of
phenol degradation under simulated solar light. The obtained tungstates
and molybdates revealed excellent photocatalytic activity despite
the low surface area and wide bandgap typical for insulators. The
mechanism of phenol degradation proceeded through hydroquinone and
catechol formation in the presence of hydroxyl and superoxide radicals.
The presence of electron traps allowed absorption of light with lower
energy than resulting from the absorption edge. BaWO4 and
SrWO4, with the most extended average carrier lifetime,
were the most efficient photocatalysts from the obtained series. In
general, molybdates exhibited lower photocatalytic activity toward
phenol degradation due to deeper trap states and lower average charge
carrier lifetimes than tungstates. Additionally, electrochemical studies
demonstrated that molybdates exhibit more insulating behavior than
tungstates. The overall results showed that wide-bandgap semiconductors,
mainly tungstates, can be applied as earth-abundant photocatalytic
materials for the degradation of persistent organic pollutants.