Some glasses in the RE
2O
3–MoO
3–B
2O
3 system (RE: Gd, Sm, Dy) were prepared by using a conventional melt quenching method, and the self-powdering phenomenon of β′-Gd
2(MoO
4)
3 crystals, i.e., the breaking into small pieces during the crystal growth, was examined using polarized optical microscope observations in a heating stage. In Gd
2O
3–MoO
3–B
2O
3 glasses with Gd
2O
3/MoO
3 = 1/3 and with different B
2O
3 contents (15–30 mol %) such as 20Gd
2O
3–60MoO
3–20B
2O
3, β′-Gd
2(MoO
4)
3 crystals were formed and the self-powdering phenomenon was observed irrespective of B
2O
3 content. The crack formation radiating out from the center part was clearly observed in the inside of crystals (diameter >40 µm) formed at 570°C in the glasses with Gd
2O
3 or Dy
2O
3. But, any clear crack formation was not observed in the glass with Sm
2O
3. It was found that the base glasses have larger densities at room temperature compared with β′-RE
2(MoO
4)
3 crystals formed, which is a unique feature in the RE
2O
3–MoO
3–B
2O
3 system compared with the crystallization of other glass systems. Such differences in the density might induce the accumulation of extremely large stresses in the inside of crystals, eventually causing the breaking of crystals.
抄録全体を表示