Solid solutions of BiGa
xM1鈥?i>xO
3 (
M = Cr, Mn, and Fe) were prepared using the high-pressure high-temperature method at 6 GPa and 1700 K (
M = Cr and Fe) and 1300 K (
M = Mn). The formation of a large family of polar materials with
R3
c and
Cm symmetries was found. Crystal structures were studied with laboratory X-ray powder diffraction: space group
Cm,
a = 5.3150(1) 脜,
b = 5.2960(1) 脜,
c = 4.6965(1) 脜, and 尾 = 92.556(2)掳 for BiGa
0.4Fe
0.6O
3; space group
Cm,
a = 5.2798(1) 脜,
b = 5.2577(1) 脜,
c = 4.6465(1) 脜, and 尾 = 91.974(2)掳 for BiGa
0.7Mn
0.3O
3; space group
R3
c,
a = 5.51623(8) 脜 and
c = 13.61391(17) 脜 for BiGa
0.4Cr
0.6O
3. Samples with the
Cm symmetry have square-pyramidal coordination of (Ga,
M)
3+ ions, and their structure is very similar with the structure of supertetragonal PbVO
3, BiCoO
3, and Bi
2ZnTiO
6 materials. Samples with the
R3
c symmetry are isostructural with BiFeO
3 and have comparable calculated (based on the point-charge model) spontaneous polarization (58 渭C/cm
2 for BiGa
0.4Cr
0.6O
3). The calculated polarization is 116 渭C/cm
2 for BiGa
0.4Fe
0.6O
3, and 102 渭C/cm
2 for BiGa
0.7Mn
0.3O
3. BiGa
0.4Cr
0.6O
3 has a first-order structural phase transition at 850 K, and other polar samples showed no phase transitions below decomposition temperatures. The BiGa
xMn
1鈥?i>xO
3 system demonstrated strong phase competition at 0.6 鈮?
x 鈮?2/3.
Keywords:
perovskites; multiferroics; high-pressure; supertetragonality; BiFeO3