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Design principles of perovskites for solar-driven thermochemical splitting of CO₂
- Ezbiri, Miriam, Takacs, Michael, Stolz, Boris, Lungthok, Jeffrey, Steinfeld, Aldo, Michalsky, Ronald
- Journal of materials chemistry A 2017 v.5 no.29 pp. 15105-15115
- Gibbs free energy, X-ray diffraction, carbon dioxide, carbon monoxide, carbonates, chemical composition, electrochemistry, enthalpy, fuels, metal ions, oxidation, oxygen, phase transition, temperature, thermogravimetry, transmission electron microscopy
- Perovskites are attractive redox materials for thermo/electrochemical fuel synthesis. To design perovskites with balanced redox energetics for thermochemically splitting CO₂, the activity of lattice oxygen vacancies and stability against crystal phase changes and detrimental carbonate formation are predicted for a representative range of perovskites by electronic structure computations. Systematic trends in these materials properties when doping with selected metal cations are described in the free energy range defined for isothermal and temperature-swing redox cycles. To confirm that the predicted materials properties root in the bulk chemical composition, selected perovskites are synthesized and characterized by X-ray diffraction, transmission electron microscopy, and thermogravimetric analysis. On one hand, due to the oxidation equilibrium, none of the investigated compositions outperforms non-stoichiometric ceria – the benchmark redox material for CO₂ splitting with temperature-swings in the range of 800–1500 °C. On the other hand, certain promising perovskites remain redox-active at relatively low oxide reduction temperatures at which ceria is redox-inactive. This trade-off in the redox energetics is established for YFeO₃, YCo₀.₅Fe₀.₅O₃ and LaFe₀.₅Ni₀.₅O₃, identified as stable against phase changes and capable to convert CO₂ to CO at 600 °C and 10 mbar CO in CO₂, and to being decomposed at 1400 °C and 0.1 mbar O₂ with an enthalpy change of 440–630 kJ mol⁻¹ O₂.