Sol–gel derived CuCoMnOx spinel coatings for solar absorbers: Structural and optical properties

Abstract A novel black coloured coating with the composition CuCoMnO x was prepared using sol–gel synthesis. The coatings were deposited using the dip-coating technique from alcoholic sols based on Mn-acetate and Co- and Cu-chloride precursors. Thermogravimetric analysis showed that xerogels become crystalline at 316°C while X-ray diffraction analysis revealed that the coatings and powders correspond predominantly to CuCoMnO x spinels. Rutherford back scattering (RBS) and transmission electron microscopic (TEM) studies combined with energy dispersive X-ray spectroscopy (EDXS) measurements confirmed that Cu, Mn and Co are present in the films in stoichiometric ratios close to that in the initial sols. IR spectroscopy has been employed to study the formation of sols by following the changes in the vibrational bands of the acetate groups during both thermal hydrolysis and the ageing of sols to xerogels. It was found that ageing of xerogels was accompanied by the formation of −COO − bridging units, which at 250°C are no longer visible in the IR spectra but substituted by the vibrational modes characteristic for CuCoMnO x . The solar absorptance ( a s ) and thermal emittance ( e T ) of the coatings when deposited on an Al-substrate are a s =0.9 and e T =0.05, which rank deposited black sol–gel CuCoMnO x spinels among the promising candidates for spectrally selective absorber coatings for solar collectors and solar facades.