Sintering and Grain Growth of Rare Earth-Doped Ceria Particles

  • Sameshima, Soichiro (Department of Applied Chemistry and Chemical Engineering, Kagoshima University) ;
  • Higashi, Kenji (Department of Applied Chemistry and Chemical Engineering, Kagoshima University) ;
  • Hirata, Yoshihiro (Department of Applied Chemistry and Chemical Engineering, Kagoshima University)
  • 발행 : 2000.06.01

초록

Rare earth-doped ceria powders with a composition of Ce0.8R0.2O1.9(R=Yb, Y, Gd, Sm, Nd and La) were prepared by heating the oxalate coprecipitate. The green compacts began to shrink at 600$^{\circ}$-700$^{\circ}C$. The relative density after the sintering at 1200$^{\circ}$ and 1400$^{\circ}C$ became higher for the higher green density. The samples were densified above 98% relative density by the sintering ant 1600$^{\circ}C$ for 4 h and the grain sizes (4.7-7.6$\mu\textrm{m}$) showed a tendency to become larger with increasing ionic radius of doped-rare earth element. In the intial stag of sintering at 700$^{\circ}$-800$^{\circ}C$, the dominant mass transport process changed from lattice diffusion to grain boundary diffusion to grain boundary diffusion with heating time. The porosity during the intermediated and final stage of the sintering at 1200$^{\circ}$ and 1400$^{\circ}C$ decreased by the mass transport through lattice diffusion with grain growth.

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