Crystal Growth and Phase Formation of High-Entropy Rare-Earth Aluminum Perovskites

Matheus Pianassola, Bryan C. Chakoumakos, Charles L. Melcher, Mariya Zhuravleva

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

We demonstrate for the first time the crystal growth of high-entropy rare-earth (RE) aluminum perovskites (REAlO3) using the micro-pulling-down method to inform future exploration of functional crystals. To determine how composition affects phase formation, we formulate equiatomic compositions containing five REs from the following list: Lu, Yb, Tm, Er, Y, Ho, Dy, Tb, Gd, Eu, Sm, Nd, Pr, Ce, La. To test whether combinations of REs with similar ionic radii may favor a single phase, compositions containing REs with consecutive or nonconsecutive ionic radius values were formulated. Powder and single-crystal X-ray diffraction indicate that crystals containing only REs with similar ionic radii that form orthorhombic single-RE REAlO3 are a single phase. Crystals containing REs with dissimilar ionic radii or mixtures of REs that form orthorhombic, rhombohedral, and tetragonal single-RE REAlO3 are a mixture of phases. The elemental distribution in single-phase crystals analyzed via electron probe microanalysis confirms no evidence of preferential incorporation of any of the constituent REs. The distribution and composition of secondary phases were analyzed via scanning electron microscopy and energy dispersive spectroscopy; secondary phases were seen as a small region in the center of the crystals with branching features closer to the outer surface.

Original languageEnglish
Pages (from-to)480-488
Number of pages9
JournalCrystal Growth and Design
Volume23
Issue number1
DOIs
StatePublished - Jan 4 2023

Funding

This work was supported by the National Science Foundation (DMR 1846935). Powder XRD was performed at the Institute for Advanced Materials & Manufacturing (IAMM) Diffraction Facility, located at the University of Tennessee, Knoxville. Electron microprobe measurements were performed at the Electron Microprobe Laboratory in the Department of Earth and Planetary Sciences at the University of Tennessee, Knoxville with the assistance of Molly McCanta and Allan Patchen. A portion of this research used resources at the Spallation Neutron Source, a Department of Energy Office of Science User Facility operated by the Oak Ridge National Laboratory.

FundersFunder number
Department of Earth and Planetary Sciences at the University of Tennessee
Institute for Advanced Materials & Manufacturing
National Science FoundationDMR 1846935
Office of Science
Oak Ridge National Laboratory
University of Tennessee

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