RESUMO
We report on the experimental demonstration of an aerosol solar reactor for the thermal reduction of ceria, as part of a thermochemical redox cycle for splitting H2O and CO2. The concept utilizes a cavity-receiver enclosing an array of alumina tubes, each containing a downward gravity-driven aerosol flow of ceria particles countercurrent to an inert sweep gas flow for intrinsic separation of reduced ceria and oxygen. A 2 kWth lab-scale prototype with a single tube was tested under radiative fluxes approaching 4000 suns, yielding reaction extents of up to 53% of the thermodynamic equilibrium at 1919 K within residence times below 1 s. Upon thermal redox cycling, fresh primary particles of 2.44 µm mean size initially formed large agglomerates of 1000 µm mean size, then sintered into stable particles of 150 µm mean size. The reaction extent was primarily limited by heat transfer for large particles/agglomerates (mean size > 200 µm) and by the gas phase advection of product O2 for smaller particles.
