Study of Oxygen Vacancies in Ce0.9Pr0.1O2-δ Solid Solution by in Situ X-ray Diffraction and in Situ Raman Spectroscopy

A Ce 0.9 Pr 0.1 O 2- δ solid solution was prepared by a sol−gel method. Changes in microstructure of the solid solution under different atmospheres (O 2, He, and H 2 ) and temperatures were characterized by an in situ X-ray diffraction (XRD) technique. Raman peaks at 460 cm -1 ascribed to the F 2g vibration mode of CeO 2 in the fluorite structure and at 570 cm -1 ascribed to oxygen vacancies in the solid solution were studied by in situ Raman spectroscopy using 785- and 514-nm excitation laser lines, providing bulk and surface information, respectively. With a 785-nm laser line, the A 570 / A 460 ratio reflecting the oxygen vacancies concentration increased under O 2 and He while it first increased and then decreased under H 2 with increasing temperature. With a 514-nm excitation laser line, the A 570 / A 460 ratio decreased with increasing temperature under all atmospheres. The growth of the A 570 / A 460 ratio under the 785-nm laser line was due to the positive effects of high temperature and high concentration of oxygen vacancies and the negative effect of reduction of the sample under reducing atmospheres (He and H 2 ), while the decline in the A 570 / A 460 ratio under 514 nm was due to the dominant negative effect of the migration of surface Pr from surface to bulk during the heating process.