Apr 26, 2024
4:00pm - 4:15pm
Room 335, Level 3, Summit
Irene Martin1,2,Luca Rebecchi1,3,Andrea Rubino1,Ilka Kriegel1
Istituto Italiano di Tecnologia1,Politecnico di Torino2,Università degli Studi di Genova3
Irene Martin1,2,Luca Rebecchi1,3,Andrea Rubino1,Ilka Kriegel1
Istituto Italiano di Tecnologia1,Politecnico di Torino2,Università degli Studi di Genova3
Dark photocatalysis is a promising technology for fuel production, which combines light harvesting properties with energy storing materials. The system involved would both work as a photocatalyst and rechargeable solar battery under illumination, so that electrons released during the discharge could be exploited for ‘dark’ reactions, <i>e.g.</i> CO<sub>2</sub> reduction reaction (CO<sub>2</sub>RR) and hydrogen evolution reaction (HER). Thus, it also implies the investigation of materials capable of storing electrons for hours [1]. Tungsten(III) oxide (WO<sub>3</sub>) has drawn interest owing to its ability of trapping electrons through intercalation of positive ions, accommodating negative charges at W centres [2], and being utilised for prolonged anti-corrosion activity in the dark (<i>i.e.</i> photocathodic protection) [3].<br/>In the work herein presented we investigated the potential use of WO<sub>3</sub> nanoparticles for dark photocatalytic CO<sub>2</sub>RR by means of photo-doping process. We analyzed the charge storing properties of the WO<sub>3</sub> colloidal nanoparticles via UV-VIS-NIR spectroscopy, by monitoring absorption changes under illumination. The increase of the LSPR peak and the blue shift of the band gap due to the Moss-Burstein effect indicate that WO<sub>3</sub> undergoes electron accumulation, similar to what has already been reported for indium tin oxide (ITO) and other metal oxide nanocrystals (MO NCs) [4]. The results obtained in our study suggest that these materials can be valid candidates for next generation of photocatalytic systems.<br/><br/>[1] Rogolino and Savateev, <i>Adv. Funct. Mater</i> <b>2023</b> 2305028<br/>[2] Ng et al., <i>Phys. Chem. Chem. Phys</i> <b>2011</b> 13 13421-13426<br/>[3] Zhou et al., <i>Corros. Sci.</i> <b>2009</b> 51 1386-1391<br/>[4] Ghini <i>et al.</i>, <i>Nanoscale </i><b>2021</b> 19 8773-8783