Structure and microstructure of Sm xY 2− xO 3

Abstract

Sm x Y 2− x O 3 solid solutions are semimagnetic semiconducting materials with wide energy gaps. Magnetic properties of these materials are coupled with their structural and microstructural parameters. Evidently, it is of interest to investigate these parameters in order to explain magnetic properties of diluted magnets. All mixed sesquioxides Sm x Y 2− x O 3 ( x = 0.2, 0.5, 0.7, 1.0, 1.4 and 1.7) crystallize in C-M 2O 3 crystaltype in space group Ia3 with Y 3+ and Sm 3+ cations in 24(d) and 8(b) Wyckoff positions, respectively. The X-ray diffraction data were used to establish the distribution of magnetic ions over crystallographic positions 8(b) and 24(d). A random distribution was found. The same data were used for evaluation of the crystal size, microstrain and paracrystallinity. The concentration dependence of these values was concluded. Results show that unit cell parameters obey Vegard's rule. That fact leads to indirect information about well mixing of Y 2O 3 and Sm 2O 3. Agreement of the unit cell parameters with Vegard's rule is connected with the difference between cationic radii and electronegativity. The Sm 3+O 2−Sm 3+ bond geometry, important for the superexchange interaction, strongly depends on Sm 3+ concentration. By comparing difference of unit cell parameters of the constitutive components Y 2O 3 and Sm 2O 3 and values of microstrains of their solid solutions it can be concluded that clusters are randomly formed.