{110}-Layered B-cation ordering in the anion-deficient perovskite Pb 2.4 Ba 2.6 Fe 2 Sc 2 TiO 13 with the crystallographic shear structure
A novel anion-deficient perovskite-based compound, Pb 2.4 Ba 2.6 Fe 2 Sc 2 TiO 13 , was synthesized via the citrate-based route. This compound is an n = 5 member of the A n B n O 3n−2 homologous series with unit-cell parameters related to the perovskite subcell a p ≈ 4.0 Å as a p √2 × a p × 5 a p √2...
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Veröffentlicht in: | Dalton transactions : an international journal of inorganic chemistry 2015, Vol.44 (23), p.10753-10762 |
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Sprache: | eng |
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Zusammenfassung: | A novel anion-deficient perovskite-based compound, Pb
2.4
Ba
2.6
Fe
2
Sc
2
TiO
13
, was synthesized
via
the citrate-based route. This compound is an
n
= 5 member of the A
n
B
n
O
3n−2
homologous series with unit-cell parameters related to the perovskite subcell
a
p
≈ 4.0 Å as
a
p
√2 ×
a
p
× 5
a
p
√2. The crystal structure of Pb
2.4
Ba
2.6
Fe
2
Sc
2
TiO
13
consists of quasi-2D perovskite blocks with a thickness of three octahedral layers separated by the 1/2[110](1̄01)
p
crystallographic shear (CS) planes, which are parallel to the {110} plane of the perovskite subcell. The CS planes transform the corner-sharing octahedra into chains of edge-sharing distorted tetragonal pyramids. Using a combination of neutron powder diffraction,
57
Fe Mössbauer spectroscopy and atomic resolution electron energy-loss spectroscopy we demonstrate that the B-cations in Pb
2.4
Ba
2.6
Fe
2
Sc
2
TiO
13
are ordered along the {110} perovskite layers with Fe
3+
in distorted tetragonal pyramids along the CS planes, Ti
4+
preferentially in the central octahedra of the perovskite blocks and Sc
3+
in the outer octahedra of the perovskite blocks. Magnetic susceptibility and Mössbauer spectroscopy indicate a broadened magnetic transition around
T
N
∼ 45 K and the onset of local magnetic fields at low temperatures. The magnetic order is probably reminiscent of that in other A
n
B
n
O
3n−2
homologues, where G-type AFM order within the perovskite blocks has been observed. |
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ISSN: | 1477-9226 1477-9234 |
DOI: | 10.1039/C4DT03867C |