Grain growth has been characterized for various zirconia alloys and ca
tion segregations have been measured with AES and ESCA. The samples we
re prepared by coprecipitation, followed by compacting and sintering a
t 1400 degrees C for different times. Grain growth was found to depend
strongly on the dopants, e.g. on their radius and valence state. Howe
ver; segregation factors of these cations did not reveal significant d
ifferences. Impurities up to 1 wt% are found to control grain growth v
ia a grain boundary layer. Large amounts of Cr2O3 and SnO2 tend to sup
press grain growth effectively by the spherical shaped precipitations.
The results are discussed in relation to the existing grain growth mo
dels.