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High Hydrostatic Pressure (0.5–2.5 GPa) Synthesis and Properties of Bulk “<i>nnx</i>” Rare-Earth Nickel Oxides (<i>R<sub>n</sub></i>Ni<i><sub>n</sub></i>O<i><sub>x</sub></i>)*

ORAL

Abstract

We have undertaken rare-earth and alkaline-earth substitutions in known nickel oxide phases, and a search for new such phases, using a hot press. We prepared starting materials both by ambient solid-state reaction (650°C–975°C) and by using high-oxygen-pressure (150–200 bar), high-temperature (T ≈ 1000°C) syntheses, producing either nominal-composition mixed-phase RNiOx materials, or the nearly-simple-perovskite RNiO3 phases, respectively. We then subjected such parent materials [R = Pr, Nd, (La,Y)], as well as hole- and electron-doped varieties, to high quasi-hydrostatic pressures using a hot piston-cylinder apparatus (5–25 kbar, i.e., 0.5–2.5 GPa) at high temperatures (950°C–1050°C). The technique1 can include oxidizers (KClO4), or can be naturally reducing, the latter augmentable by hydrogen. We report product phases; initial syntheses have provided specimens with decreases in undesired starting phases. Our study of other nickelate phases, e.g., R3Ni3O7 and infinite-layer RNiO2, with this technique is ongoing, exploring both steric effects and hole- (Sr2+) and electron-doping (Ce4+) in targeted RnNinOx structures.
1G. Démazeau et al., J. Solid State Chem. 3, 582 (1971).

Presenters

  • Sara J Irvine

    Department of Physics, University of Texas at Austin

Authors

  • Sara J Irvine

    Department of Physics, University of Texas at Austin

  • Gregorio Ponti

    Department of Physics, University of Texas at Austin

  • Quinn D. B. Timmers

    Department of Physics, University of Texas at Austin

  • Zachary P. Kuklinski

    Department of Physics, University of Texas at Austin

  • John T. Markert

    Department of Physics, University of Texas at Austin, Department of Physics, The University of Texas at Austin