Abstract
We investigate how grain growth, strain relaxation, and vacancy chemistry shape the near-edge optical response of nanocrystalline CeO prepared by a chymosin-assisted Pechini route from nitrate–citrate precursors. Rietveld line-profile analysis shows that phase-pure CeO forms after calcination between 400 and 1000 C. Over this range, the average crystallite size increases from ≈3.4 to ≈57 nm, while the microstrain decreases from 0.79% to 0.05%, with size–strain scaling consistent with interface-controlled grain growth that follows a normal growth law with exponent and activation energy kJ mol . Raman spectroscopy tracks the sharpening of the mode and the fading of defect-related bands, X-ray photoelectron spectroscopy reveals a nonmonotonic evolution of the surface Ce fraction and separates lattice from adsorbed oxygen species, and electron paramagnetic resonance detects vacancy-bound Ce polarons that weaken at high temperature. Diffuse-reflectance UV–Vis spectra show a modest blue shift of the apparent band gap from to 2.95 eV as crystallites coarsen, while the Urbach energy follows the Ce content and sub-gap tailing. The structural, spectroscopic, and optical results together map out a quantitative connection between grain growth, vacancy populations, and near-edge optical properties in CeO nanoparticles.