5 research outputs found

    Postperovskite Phase Transition of ZnGeO<sub>3</sub>: Comparative Crystal Chemistry of Postperovskite Phase Transition from Germanate Perovskites

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    The postperovskite phase of ZnGeO<sub>3</sub> was confirmed by laser heating experiments of the perovskite phase under 110–130 GPa at high temperature. Ab initio calculations indicated that the phase transition occurs at 133 GPa at 0 K. This postperovskite transition pressure is significantly higher than those reported for other germanates, such as MnGeO<sub>3</sub> and MgGeO<sub>3</sub>. The comparative crystal chemistry of the perovskite-to-postperovskite transition suggests that a relatively elongated <i>b</i>-axis in the low-pressure range resulted in the delay in the transition to the postperovskite phase. Similar to most GdFeO<sub>3</sub>-type perovskites that transform to the CaIrO<sub>3</sub>-type postperovskite phase, ZnGeO<sub>3</sub> perovskite eventually transformed to the CaIrO<sub>3</sub>-type postperovskite phase at a critical rotational angle of the GeO<sub>6</sub> octahedron. The formation of the postperovskite structure at a very low critical rotational angle for MnGeO<sub>3</sub> suggests that relatively large divalent cations likely break down the corner-sharing GeO<sub>6</sub> frameworks without a large rotation of GeO<sub>6</sub> to form the postperovskite phase

    High-Pressure Synthesis, Crystal Structure, and Phase Stability Relations of a LiNbO<sub>3</sub>‑Type Polar Titanate ZnTiO<sub>3</sub> and Its Reinforced Polarity by the Second-Order Jahn–Teller Effect

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    A polar LiNbO<sub>3</sub>-type (LN-type) titanate ZnTiO<sub>3</sub> has been successfully synthesized using ilmenite-type (IL-type) ZnTiO<sub>3</sub> under high pressure and high temperature. The first principles calculation indicates that LN-type ZnTiO<sub>3</sub> is a metastable phase obtained by the transformation in the decompression process from the perovskite-type phase, which is stable at high pressure and high temperature. The Rietveld structural refinement using synchrotron powder X-ray diffraction data reveals that LN-type ZnTiO<sub>3</sub> crystallizes into a hexagonal structure with a polar space group <i>R</i>3<i>c</i> and exhibits greater intradistortion of the TiO<sub>6</sub> octahedron in LN-type ZnTiO<sub>3</sub> than that of the SnO<sub>6</sub> octahedron in LN-type ZnSnO<sub>3</sub>. The estimated spontaneous polarization (75 μC/cm<sup>2</sup>, 88 μC/cm<sup>2</sup>) using the nominal charge and the Born effective charge (BEC) derived from density functional perturbation theory, respectively, are greater than those of ZnSnO<sub>3</sub> (59 μC/cm<sup>2</sup>, 65 μC/cm<sup>2</sup>), which is strongly attributed to the great displacement of Ti from the centrosymmetric position along the <i>c</i>-axis and the fact that the BEC of Ti (+6.1) is greater than that of Sn (+4.1). Furthermore, the spontaneous polarization of LN-type ZnTiO<sub>3</sub> is greater than that of LiNbO<sub>3</sub> (62 μC/cm<sup>2</sup>, 76 μC/cm<sup>2</sup>), indicating that LN-type ZnTiO<sub>3</sub>, like LiNbO<sub>3</sub>, is a candidate ferroelectric material with high performance. The second harmonic generation (SHG) response of LN-type ZnTiO<sub>3</sub> is 24 times greater than that of LN-type ZnSnO<sub>3</sub>. The findings indicate that the intraoctahedral distortion, spontaneous polarization, and the accompanying SHG response are caused by the stabilization of the polar LiNbO<sub>3</sub>-type structure and reinforced by the second-order Jahn–Teller effect attributable to the orbital interaction between oxygen ions and d<sup>0</sup> ions such as Ti<sup>4+</sup>

    High-Pressure Synthesis, Crystal Structure, and Electromagnetic Properties of CdRh<sub>2</sub>O<sub>4</sub>: an Analogous Oxide of the Postspinel Mineral MgAl<sub>2</sub>O<sub>4</sub>

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    The postspinel mineral MgAl<sub>2</sub>O<sub>4</sub> exists only under the severe pressure conditions in the subducted oceanic lithosphere in the Earth’s deep interior. Here we report that its analogous oxide CdRh<sub>2</sub>O<sub>4</sub> exhibits a structural transition to a quenchable postspinel phase under a high pressure of 6 GPa at 1400 °C, which is within the general pressure range of a conventional single-stage multianvil system. In addition, the complex magnetic contributions to the lattice and metal nonstoichiometry that often complicate investigations of other analogues of MgAl<sub>2</sub>O<sub>4</sub> are absent in CdRh<sub>2</sub>O<sub>4</sub>. X-ray crystallography revealed that this postspinel phase has an orthorhombic CaFe<sub>2</sub>O<sub>4</sub> structure, thus making it a practical analogue for investigations into the geophysical role of postspinel MgAl<sub>2</sub>O<sub>4</sub>. Replacement of Mg<sup>2+</sup> with Cd<sup>2+</sup> appears to be effective in lowering the pressure required for transition, as was suggested for CdGeO<sub>3</sub>. In addition, Rh<sup>3+</sup> could also contribute to this reduction, as many analogous Rh oxides of aluminous and silicic minerals have been quenched from lower-pressure conditions

    High-Pressure Synthesis of 5d Cubic Perovskite BaOsO<sub>3</sub> at 17 GPa: Ferromagnetic Evolution over 3d to 5d Series

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    In continuation of the series of perovskite oxides that includes 3d<sup>4</sup> cubic BaFeO<sub>3</sub> and 4d<sup>4</sup> cubic BaRuO<sub>3</sub>, 5d<sup>4</sup> cubic BaOsO<sub>3</sub> was synthesized by a solid-state reaction at a pressure of 17 GPa, and its crystal structure was investigated by synchrotron powder X-ray diffraction measurements. In addition, its magnetic susceptibility, electrical resistivity, and specific heat were measured over temperatures ranging from 2 to 400 K. The results establish a series of d<sup>4</sup> cubic perovskite oxides, which can help in the mapping of the itinerant ferromagnetism that is free from any complication from local lattice distortions for transitions from the 3d orbital to the 5d orbital. Such a perovskite series has never been synthesized at any d configuration to date. Although cubic BaOsO<sub>3</sub> did not exhibit long-range ferromagnetic order unlike cubic BaFeO<sub>3</sub> and BaRuO<sub>3</sub>, enhanced feature of paramagnetism was detected with weak temperature dependence. Orthorhombic CaOsO<sub>3</sub> and SrOsO<sub>3</sub> show similar magnetic behaviors. CaOsO<sub>3</sub> is not as conducting as SrOsO<sub>3</sub> and BaOsO<sub>3</sub>, presumably due to impact of tilting of octahedra on the width of the <i>t</i><sub>2g</sub> band. These results elucidate the evolution of the magnetism of perovskite oxides not only in the 5d system but also in group 8 of the periodic table

    Synthesis, Crystal Structure, and Electronic Properties of High-Pressure PdF<sub>2</sub>‑Type Oxides MO<sub>2</sub> (M = Ru, Rh, Os, Ir, Pt)

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    The polycrystalline MO<sub>2</sub>’s (HP-PdF<sub>2</sub>-type MO<sub>2</sub>, M = Rh, Os, Pt) with high-pressure PdF<sub>2</sub> compounds were successfully synthesized under high-pressure conditions for the first time, to the best of our knowledge. The crystal structures and electromagnetic properties were studied. Previously unreported electronic properties of the polycrystalline HP-PdF<sub>2</sub>-type RuO<sub>2</sub> and IrO<sub>2</sub> were also studied. The refined structures clearly indicated that all compounds crystallized into the HP-PdF<sub>2</sub>-type structure, M<sup>4+</sup>O<sup>2–</sup><sub>2</sub>, rather than the pyrite-type structure, M<sup><i>n</i>+</sup>(O<sub>2</sub>)<sup><i>n</i>−</sup> (<i>n</i> < 4). The MO<sub>2</sub> compounds (M = Ru, Rh, Os, Ir) exhibited metallic conduction, while PtO<sub>2</sub> was highly insulating, probably because of the fully occupied t<sub>2g</sub> band. Neither superconductivity nor a magnetic transition was detected down to a temperature of 2 K, unlike the case of 3d transition metal chalcogenide pyrites
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