Combining partial
oxidation of methane with H2O/CO2 splitting
under solar thermal conditions presents a very
promising strategy for producing solar fuels. In order to achieve
this, the development of stable and efficient redox catalysts is necessary,
among which ceria (CeO2) seems to be one of the most promising
for lattice oxygen transfer. In this study, CeO2 was used
for splitting CO2 and H2O using concentrated
solar energy with reaction temperatures in the range 900–1100
°C. The experimental studies in a solar-driven thermogravimetric
system indicated that both CH4 induced reduction and CO2 induced oxidation of CeO2−δ followed
close reaction orders with activation energies of 109 and 36 kJ mol–1, respectively. The results were compared with those
obtained from hydrothermal templating and surfactant induced self-assembly.
To our knowledge, such materials are studied for the first time for
CH4 induced fuel production via solar thermochemical redox
cycles. Enhanced reaction rates and stability upon cycling were observed
for materials synthesized by hydrothermal and self-assembly methods.
Experiments were also carried out to deduce the effect of various
inert materials (MgO and Al2O3) as promotional
agents. Higher reduction rate and maximum nonstoichiometry (δ
= 0.431) during reduction at 1000 °C were observed in the case
of MgO promoted CeO2. In addition, the amount of evolved
CO was found to be the highest (δ = 0.402), indicating almost
complete reoxidation. The achieved nonstoichiometry and the resulting
fuel productivity are more than 10 times higher than the reported
values for thermal reduction of ceria. Studies were also performed
in a solar reactor prototype, enabling both partial ceria reduction
with methane, followed by oxidation with H2O/CO2. Typically, MgO and Al2O3 promoted ceria were
tested under packed bed conditions and compared with commercial ceria
for syngas production. In this case, significant enhancement in the
system efficiency was observed for MgO promoted CeO2.