Binary compounds in the systems Ln
2O
3-Ga
2O
3 (Ln=La, Pr, Nd, Sm, Eu, Gd, Dy, Ho, Er, Yb) were studied by solid state reaction and a quenching technique using a heliostat-type solar furnace. In the systems, the existence of four types of compounds was shown; garnet-type 3Ln
2O
3⋅5Ga
2O
3 (Ln=Nd, Sm, Eu, Gd, Dy, Ho, Er, Yb), perovskite-type LnGaO
3 (Ln=La, Pr, Nd), monoclinic 2Ln
2O
3⋅Ga
2O
3 (Ln=La, Pr, Nd, Sm, Eu, Gd) and orthorhombic 3Ln
2O
3⋅Ga
2O
3 (Ln=Sm, Eu, Gd, Dy, Ho, Er). These binary compounds, except LaGaO
3, showed no phase transition during repeated heating and cooling cycles. In LaGaO
3, a reversible orthorhombic-rhombohedral transition was found to occur at about 900°C, using a high-temperature X-ray diffractometer. Most of the binary compounds melted congruently. With increase in the ionic radius of Ln, the solidification point decreased for LnGaO
3-type compounds and increased for 3Ln
2O
3⋅5Ga
2O
3-type and 2Ln
2O
3⋅Ga
2O
3-type compounds. Meanwhile, 3Ln
2O
3⋅Ga
2O
3-type compounds and 2Gd
2O
3⋅Ga
2O
3 were found to melt incongruently. The lattice parameters for the compounds showed shrinkage with the decrease of ionic radii of Ln. The refractive indices of the binary compounds were measured as follows:
n=2.01-2.04 for 3Ln
2O
3⋅5Ga
2O
3,
nγ=2.05-2.06,
nα=2.04-2.05 for LnGaO
3,
nγ=1.95-2.01,
nα=1.93-1.99 for 2 Ln
2O
3⋅Ga
2O
3, and
nγ=2.01-2.05,
nα=2.00-2.02 for 3Ln
2O
3⋅Ga
2O
3.
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