Thermochemical splitting of CO2 using solution combustion synthesized lanthanum-strontium-manganese perovskites

Redox reactivity of La(1-x)SrxMnO3 (LSM) perovskites towards a solar thermochemical CO2 splitting (CS) cycle is investigated. The LSM perovskites are synthesized via a solution combustion synthesis (SCS) method using glycine as the reducing agent. Multiple analytical techniques are used for the structural characterization of the LSM perovskites. Thermogravimetric thermal reduction (TR) and CS cycles (in three sets: one, three and ten cycles) are conducted to estimate the amounts of O-2 released (n(O2)) and CO produced (nCO) by each LSM perovskite. Higher n(O2) by each LSM perovskite, as compared to the nCO during the first cycle. The n(O2) is decreased, and the re-oxidation capacity of each LSM perovskite is improved from cycle one to three. In terms of the average n(O2) and nCO from cycle 2 to cycle 10, the La0.60Sr0.41Mn0.99O2.993 (214.8 mu mol of O2/g.cycle) and La0.30Sr0.70Mn0.99O2.982 perovskites (342.1 mu mol of CO/g.cycle) are observed to have the uppermost redox reactivity. The redox reactivity of all the LSM perovskites (except for La0.88Sr0.11Mn1.00O2.980) is recorded to be higher than that of the widely studied CeO2 material.

Automated summary

The redox reactivity of La(1-x)SrxMnO3 (LSM) perovskites towards a solar thermochemical CO2 splitting (CS) cycle was investigated. The LSM perovskites showed higher oxygen release and CO production compared to widely studied CeO2 material, with La0.60Sr0.41Mn0.99O2.993 and La0.30Sr0.70Mn0.99O2.982 perovskites exhibiting the highest redox reactivity.