65 research outputs found
Anisotropic Thermal Expansion and a Second-Order Charge Order Transition in the Ferrimagnetic Dy<sub>2</sub>CuZnMn<sub>4</sub>O<sub>12</sub> Perovskite with Triple A‑Site Cation Ordering
Dy2CuZnMn4O12 perovskite, belonging
to the A-site columnar-ordered quadruple perovskite family with the
general composition of A2A′A″B4O12, was prepared by a high-pressure, high-temperature
method at 6 GPa and 1500 K. Its crystal structure was studied by synchrotron
powder X-ray diffraction between 100 and 800 K. The ideal cation distribution
(without antisite disorder) was found to be realized within the sensitivity
of the synchrotron X-ray diffraction method. Between 100 and 400 K,
it crystallizes in space group Pmmn (no. 59) and
has layered charge ordering of Mn3+ and Mn4+ at the B sites. Above 425 K, it crystallizes in space group P42/nmc (no. 137) with one crystallographic
B site and an average Mn3.5+ oxidation state. The charge
ordering transition (at TCO = 425 K) appears
to be of the second order as no anomalies were found on differential
scanning calorimetry curves and temperature dependence of the unit
cell volume, and the orthorhombic a and b lattice parameters merge gradually. The compound demonstrates anisotropic
thermal expansion with the c lattice parameter decreasing
with increasing temperature above 280 K. A ferrimagnetic transition
occurs at TC = 116 K with an additional,
gradual rise of magnetic susceptibilities below 45 K, probably due
to increases of the ordered moments of the Dy sublattices
Origin of Magnetization Reversal and Exchange Bias Phenomena in Solid Solutions of BiFeO<sub>3</sub>–BiMnO<sub>3</sub>: Intrinsic or Extrinsic?
Magnetic properties of BiFe<sub>0.7</sub>Mn<sub>0.3</sub>O<sub>3</sub> (with a Néel temperature (<i>T</i><sub>N</sub>) of 425 K) and BiFe<sub>0.6</sub>Mn<sub>0.4</sub>O<sub>3</sub> (with <i>T</i><sub>N</sub> = 350 K) were investigated
by magnetic measurements between 5 and 400 K. They crystallize in
space group <i>Pnma</i> with the √2<i>a</i><sub>p</sub> × 4<i>a</i><sub>p</sub> × 2√2<i>a</i><sub>p</sub> superstructure (<i>a</i><sub>p</sub> is the parameter of the cubic perovskite subcell) with <i>a</i> = 5.57800(9) Å, <i>b</i> = 15.7038(3) Å, and <i>c</i> = 11.22113(16) Å for BiFe<sub>0.6</sub>Mn<sub>0.4</sub>O<sub>3</sub>. Both compounds show magnetization reversal or negative
magnetization phenomena. However, it was found that the magnetization
reversal is dependent on magnetic prehistory of a sample and measurement
protocols. No magnetization reversal was observed when virgin samples
were measured below <i>T</i><sub>N</sub>. Magnetization
reversal effects appeared only when the samples were cooled in small
magnetic fields from temperatures above <i>T</i><sub>N</sub> or after the samples were magnetized. The exchange bias effect or
a shift of isothermal magnetization curves, depending on the measurement
conditions, was also observed. The exchange bias changes its sign
as a function of temperature and cooling conditions. Our findings
allowed us to propose the extrinsic origin (related to sample inhomogeneities)
of the magnetization reversal effect in these two compounds
Solid Solutions between BiMnO<sub>3</sub> and BiCrO<sub>3</sub>
Solid solutions BiMn<sub>1–<i>x</i></sub>Cr<sub><i>x</i></sub>O<sub>3</sub> (0 ≤ <i>x</i> ≤ 1) have been prepared
at 6 GPa and 1370–1620 K. Their structural properties have
been studied with synchrotron X-ray powder diffraction, and their
physical properties have been investigated by dc/ac magnetic, specific
heat, dielectric, and differential scanning calorimetry measurements.
A magnetic phase diagram of BiMn<sub>1–<i>x</i></sub>Cr<sub><i>x</i></sub>O<sub>3</sub> is established. A phase
with orbital ordering observed in BiMnO<sub>3</sub> is suppressed
at <i>x</i> > 0.1, accompanied by a drop in the ferromagnetic
Curie temperature <i>T</i><sub>C</sub> from 101 K for <i>x</i> = 0 to 76 K for <i>x</i> = 0.15 and sharp changes
in the lattice parameters. The <i>T</i><sub>C</sub> value
monotonically decreases up to <i>x</i> = 0.3 (with <i>T</i><sub>C</sub> = 53 K). For intermediate compositions with <i>x</i> = 0.4, 0.5, spin-glass magnetic properties are found at
28 and 24 K, respectively. The Néel temperature <i>T</i><sub>N</sub> linearly increases from 36 K for <i>x</i> =
0.6 to 111 K for <i>x</i> = 1.0. A spin-reorientation transition
is observed at 61 K for <i>x</i> = 0.9 and 72 K for <i>x</i> = 1.0. Re-entrant spin-glass transitions are also observed
for samples with <i>x</i> = 0.3, 0.6, 0.7 by ac susceptibility
at low temperatures. At high temperatures, a structural phase transition
from <i>C</i>2/<i>c</i> to <i>Pnma</i> symmetry is observed for all compositions with a monotonic change
of the phase transition temperature. The magnetic phase diagram from
the BiMnO<sub>3</sub>-rich side (<i>x</i> ≤ 0.5)
resembles a phase diagram of BiMn<sub>1–<i>x</i></sub>Sc<sub><i>x</i></sub>O<sub>3</sub> solid solutions, indicating
that the nature of substituting cations (magnetic or nonmagnetic)
is not crucial for doped BiMnO<sub>3</sub>
Aurivillius Phase Bi<sub>4</sub>V<sub>3</sub>O<sub>12</sub> with d<sup>1</sup> Magnetic Cations, Anisotropic and Negative Thermal Expansion, Multiple Structural Transitions, and Low-Dimensional Magnetism
Aurivillius
phases are an important class of inorganic compounds
as they often show ferroelectric properties, and some members of this
family are used in nonvolatile ferroelectric memories. The majority
of Aurivillius phases have nonmagnetic d0 cations in the
perovskite block. Bi4Ti3O12 is the
best-known and extensively studied compound within this family. Here,
using a high-pressure, high-temperature synthesis method, we could
successfully prepare a full magnetic analogue, Bi4V3O12, with d1 cations. Bi4V3O12 is unstable in air above about 520 K.
However, in an inert atmosphere, Bi4V3O12 demonstrates two first-order reversible structural transitions
near 525 and 760 K. The high-temperature prototypical phase is the
same in both Bi4V3O12 and Bi4Ti3O12 with tetragonal (T) I4/mmm symmetry and aT = 3.85608(5) Å and cT = 32.6920(8)
Å (at 850 K) for Bi4V3O12, while
the low-temperature phases are different. Bi4V3O12 shows anisotropic thermal expansion above 300 K and
negative volumetric thermal expansion above about 700 K. Magnetic
measurements showed a broad maximum near 70 K on magnetic susceptibility,
indicating the presence of low-dimensional magnetism with strong antiferromagnetic
interactions between V4+ ions with the Curie–Weiss
temperature of about −370 K. But no long-range magnetic ordering
was found in Bi4V3O12 down to 2 K
Fresh Look at the Mystery of Magnetization Reversal in YVO<sub>3</sub>
Phase transitions and detailed magnetic
properties of polycrystalline AP-YVO<sub>3.00(1)</sub> (prepared at
ambient pressure by a conventional solid-state method) and polycrystalline
HP-YVO<sub>3.04(1)</sub> and HP-YVO<sub>3.05(1)</sub> (AP-YVO<sub>3</sub> treated at 6 GPa and 1600 K during 130 and 15 min, respectively)
were investigated. The three samples showed a remarkable exchange
bias (EB) effect. HP-YVO<sub>3.04</sub> and HP-YVO<sub>3.05</sub> had
similar chemical composition, crystallographic parameters, and particle
size, but their magnetic properties were qualitatively different.
EB was negative at all temperatures in AP-YVO<sub>3</sub> and HP-YVO<sub>3.05</sub>, resulting in the absence of magnetization reversal (MR).
Positive EB was observed in HP-YVO<sub>3.04</sub> between <i>T</i><sub>N2</sub> = 71 K and <i>T</i>* = 88 K resulting
in MR or negative magnetization between those temperatures. It was
demonstrated that polycrystalline HP-YVO<sub>3.04</sub> behaved similar
to single crystals of YVO<sub>3+δ</sub>. By the careful control
of the trapped magnetic field, measurement conditions were found under
which no MR occurred in HP-YVO<sub>3.04</sub> at moderate magnetic
fields, indicating that MR is not an intrinsic property of YVO<sub>3+δ</sub>. A drastic effect of trapped magnetic fields on MR
and memory effects were observed. The importance of an “insignificant”
anomaly at <i>T</i><sub>FM</sub> = 140 K for MR was suggested.
We also suggested that “positive exchange bias”, “defects”,
“interfaces”, and “pinning” should be
keywords for understanding YVO<sub>3</sub> and probably other perovskite
materials with the MR effect
Effects of Oxygen Content on Bi<sub>3</sub>Mn<sub>3</sub>O<sub>11+δ</sub>: From 45 K Antiferromagnetism to Room-Temperature True Ferromagnetism
The effects of oxygen content on the structural, physical, and chemical properties of Bi3Mn3O11 with KSbO3-type structure have been investigated. It was found that the oxygen content in Bi3Mn3O11+δ can vary over a wide δ range, keeping the same cubic structure (space group Pn3̅, a = 9.12172(5) Å for δ = −0.5, a = 9.13784(8) Å for δ = 0, and a = 9.09863(7) Å for δ = 0.6) and semiconducting properties of the material. At the same time, magnetic properties change from true antiferromagnetic with TN = 45 K for δ = −0.5 to true ferromagnetic with TC = 307 K for δ = +0.6. Bi3Mn3O11 (δ = 0) shows ferrimagnetic-like properties with TC = 150 K and features typical for a re-entrant spin-glass below 30 K. Noticeable changes of the magnetic transition temperature and magnetism in Bi3Mn3O11+δ with δ can be compared with changes of the magnetic and electronic properties of LaMnO3+δ, BiMnO3+δ, high-temperature copper superconductors (e.g., YBa2Cu3O7+δ), and other cuprates. Bi3Mn3O11.6 shows a new record high TC among insulating/semiconducting true ferromagnets. Our results demonstrate that the oxygen content can vary for the same cation composition in KSbO3-type materials, and the oxygen content can be increased up to BiMnO3.867 (Bi3Mn3O11.6)
Effects of Oxygen Content on Bi<sub>3</sub>Mn<sub>3</sub>O<sub>11+δ</sub>: From 45 K Antiferromagnetism to Room-Temperature True Ferromagnetism
The effects of oxygen content on the structural, physical, and chemical properties of Bi3Mn3O11 with KSbO3-type structure have been investigated. It was found that the oxygen content in Bi3Mn3O11+δ can vary over a wide δ range, keeping the same cubic structure (space group Pn3̅, a = 9.12172(5) Å for δ = −0.5, a = 9.13784(8) Å for δ = 0, and a = 9.09863(7) Å for δ = 0.6) and semiconducting properties of the material. At the same time, magnetic properties change from true antiferromagnetic with TN = 45 K for δ = −0.5 to true ferromagnetic with TC = 307 K for δ = +0.6. Bi3Mn3O11 (δ = 0) shows ferrimagnetic-like properties with TC = 150 K and features typical for a re-entrant spin-glass below 30 K. Noticeable changes of the magnetic transition temperature and magnetism in Bi3Mn3O11+δ with δ can be compared with changes of the magnetic and electronic properties of LaMnO3+δ, BiMnO3+δ, high-temperature copper superconductors (e.g., YBa2Cu3O7+δ), and other cuprates. Bi3Mn3O11.6 shows a new record high TC among insulating/semiconducting true ferromagnets. Our results demonstrate that the oxygen content can vary for the same cation composition in KSbO3-type materials, and the oxygen content can be increased up to BiMnO3.867 (Bi3Mn3O11.6)
Effects of Isovalent Substitution in the Manganese Sublattice on Magnetic, Thermal, and Structural Properties of BiMnO<sub>3</sub>: BiMn<sub>1-</sub><i><sub>x</sub></i>M<i><sub>x</sub></i>O<sub>3</sub> (M = Al, Sc, Cr, Fe, Ga; 0 ≤ <i>x</i> ≤ 0.2)
Solid solutions BiMn1-xMxO3 with M = Al, Sc, Cr, Fe, and Ga and 0 ≤ x ≤ 0.2 were prepared at a high pressure
of 6 GPa and 1333−1453 K, and their magnetic, thermal, and structural properties were investigated. The orbital-ordered monoclinic phase of BiMnO3 (phase I) is destroyed by a small percentage of substitution. The M elements
can be classified by their ability to destroy phase I in the sequence Ga (x ≈ 0.08) ≈ Fe (x ≈ 0.08) x ≈ 0.04)
≈ Al (x ≈ 0.04) x ≈ 0.02), where phase I is most stable for Ga substitution (up to x ≈ 0.08) and less stable
for Sc substitution (up to x ≈ 0.02). The orbital-disordered high-temperature monoclinic phase of BiMnO3 (phase
II) is stabilized with larger x. In all cases, a compositional range was found where phases I and II coexist at room
temperature. In phase I, the effect of substitution on the ferromagnetic transition temperature is weak (e.g., TC =
102 K for BiMnO3 and TC = 99 K for BiMn0.95Ga0.05O3), but there is a drastic effect on the orbital ordering temperature
(e.g., TOO = 474 K for BiMnO3 and TOO = 412 K for BiMn0.95Ga0.05O3). Magnetic susceptibilities of phase I are
typical for ferromagnets while, in phase II, ferromagnetic cluster-glass-like behavior is observed. The magnetic
transition temperature of phase II (e.g., TC = 70 K for BiMn0.8Ga0.2O3) exhibits a sudden drop compared with that
of phase I. The effect of substitution on the structural monoclinic-to-orthorhombic transition is different depending
on M (e.g., Tstr = 768 K for BiMnO3, Tstr = 800 K for BiMn0.95Ga0.05O3, and Tstr = 738 K for BiMn0.85Cr0.15O3)
Effects of Isovalent Substitution in the Manganese Sublattice on Magnetic, Thermal, and Structural Properties of BiMnO<sub>3</sub>: BiMn<sub>1-</sub><i><sub>x</sub></i>M<i><sub>x</sub></i>O<sub>3</sub> (M = Al, Sc, Cr, Fe, Ga; 0 ≤ <i>x</i> ≤ 0.2)
Solid solutions BiMn1-xMxO3 with M = Al, Sc, Cr, Fe, and Ga and 0 ≤ x ≤ 0.2 were prepared at a high pressure
of 6 GPa and 1333−1453 K, and their magnetic, thermal, and structural properties were investigated. The orbital-ordered monoclinic phase of BiMnO3 (phase I) is destroyed by a small percentage of substitution. The M elements
can be classified by their ability to destroy phase I in the sequence Ga (x ≈ 0.08) ≈ Fe (x ≈ 0.08) x ≈ 0.04)
≈ Al (x ≈ 0.04) x ≈ 0.02), where phase I is most stable for Ga substitution (up to x ≈ 0.08) and less stable
for Sc substitution (up to x ≈ 0.02). The orbital-disordered high-temperature monoclinic phase of BiMnO3 (phase
II) is stabilized with larger x. In all cases, a compositional range was found where phases I and II coexist at room
temperature. In phase I, the effect of substitution on the ferromagnetic transition temperature is weak (e.g., TC =
102 K for BiMnO3 and TC = 99 K for BiMn0.95Ga0.05O3), but there is a drastic effect on the orbital ordering temperature
(e.g., TOO = 474 K for BiMnO3 and TOO = 412 K for BiMn0.95Ga0.05O3). Magnetic susceptibilities of phase I are
typical for ferromagnets while, in phase II, ferromagnetic cluster-glass-like behavior is observed. The magnetic
transition temperature of phase II (e.g., TC = 70 K for BiMn0.8Ga0.2O3) exhibits a sudden drop compared with that
of phase I. The effect of substitution on the structural monoclinic-to-orthorhombic transition is different depending
on M (e.g., Tstr = 768 K for BiMnO3, Tstr = 800 K for BiMn0.95Ga0.05O3, and Tstr = 738 K for BiMn0.85Cr0.15O3)
Effects of Oxygen Content on Bi<sub>3</sub>Mn<sub>3</sub>O<sub>11+δ</sub>: From 45 K Antiferromagnetism to Room-Temperature True Ferromagnetism
The effects of oxygen content on the structural, physical, and chemical properties of Bi3Mn3O11 with KSbO3-type structure have been investigated. It was found that the oxygen content in Bi3Mn3O11+δ can vary over a wide δ range, keeping the same cubic structure (space group Pn3̅, a = 9.12172(5) Å for δ = −0.5, a = 9.13784(8) Å for δ = 0, and a = 9.09863(7) Å for δ = 0.6) and semiconducting properties of the material. At the same time, magnetic properties change from true antiferromagnetic with TN = 45 K for δ = −0.5 to true ferromagnetic with TC = 307 K for δ = +0.6. Bi3Mn3O11 (δ = 0) shows ferrimagnetic-like properties with TC = 150 K and features typical for a re-entrant spin-glass below 30 K. Noticeable changes of the magnetic transition temperature and magnetism in Bi3Mn3O11+δ with δ can be compared with changes of the magnetic and electronic properties of LaMnO3+δ, BiMnO3+δ, high-temperature copper superconductors (e.g., YBa2Cu3O7+δ), and other cuprates. Bi3Mn3O11.6 shows a new record high TC among insulating/semiconducting true ferromagnets. Our results demonstrate that the oxygen content can vary for the same cation composition in KSbO3-type materials, and the oxygen content can be increased up to BiMnO3.867 (Bi3Mn3O11.6)
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