Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt

Abstract The challenge of growing rare-earth (RE) sesquioxide crystals can be overcome by tailoring their structural stability and melting point via composition engineering. This work contributes to the advancement of the field of crystal growth of high-entropy oxides. A compound with only small REs...

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Main Authors: Matheus Pianassola, Kaden L. Anderson, Joshua Safin, Can Agca, Jake W. McMurray, Bryan C. Chakoumakos, Jöerg C. Neuefeind, Charles L. Melcher, Mariya Zhuravleva
Format: Article
Language:English
Published: Tsinghua University Press 2022-08-01
Series:Journal of Advanced Ceramics
Subjects:
Online Access:https://doi.org/10.1007/s40145-022-0625-z
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author Matheus Pianassola
Kaden L. Anderson
Joshua Safin
Can Agca
Jake W. McMurray
Bryan C. Chakoumakos
Jöerg C. Neuefeind
Charles L. Melcher
Mariya Zhuravleva
author_facet Matheus Pianassola
Kaden L. Anderson
Joshua Safin
Can Agca
Jake W. McMurray
Bryan C. Chakoumakos
Jöerg C. Neuefeind
Charles L. Melcher
Mariya Zhuravleva
author_sort Matheus Pianassola
collection DOAJ
description Abstract The challenge of growing rare-earth (RE) sesquioxide crystals can be overcome by tailoring their structural stability and melting point via composition engineering. This work contributes to the advancement of the field of crystal growth of high-entropy oxides. A compound with only small REs (Lu,Y,Ho,Yb,Er)2O3 maintains a cubic C-type structure upon cooling from the melt, as observed via in-situ high-temperature neutron diffraction on aerodynamically levitated samples. On the other hand, a compound with a mixture of small and large REs (Lu,Y,Ho,Nd,La)2O3 crystallizes as a mixture of a primary C-type phase with an unstable secondary phase. Crystals of compositions (Lu,Y,Ho,Nd,La)2O3 and (Lu,Y,Gd,Nd,La)2O3 were grown by the micro-pulling-down (mPD) method with a single monoclinic B-type phase, while a powder of (Lu,Y,Ho,Yb,Er)2O3 did not melt at the maximum operating temperature of an iridium-rhenium crucible. The minimization of the melting point of the two grown crystals is attributed to the mismatch in cation sizes. The electron probe microanalysis reveals that the general element segregation behavior in the crystals depends on the composition.
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spelling doaj.art-f15d4822171a4b8883c4e1ebb24707e42023-08-02T07:19:59ZengTsinghua University PressJournal of Advanced Ceramics2226-41082227-85082022-08-011191479149010.1007/s40145-022-0625-zTuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the meltMatheus Pianassola0Kaden L. Anderson1Joshua Safin2Can Agca3Jake W. McMurray4Bryan C. Chakoumakos5Jöerg C. Neuefeind6Charles L. Melcher7Mariya Zhuravleva8Scintillation Materials Research Center, The University of TennesseeScintillation Materials Research Center, The University of TennesseeDepartment of Materials Science and Engineering, The University of TennesseeMaterials Science and Technology Division, Oak Ridge National LaboratoryMaterials Science and Technology Division, Oak Ridge National LaboratoryNeutron Scattering Division, Oak Ridge National LaboratoryNeutron Scattering Division, Oak Ridge National LaboratoryScintillation Materials Research Center, The University of TennesseeScintillation Materials Research Center, The University of TennesseeAbstract The challenge of growing rare-earth (RE) sesquioxide crystals can be overcome by tailoring their structural stability and melting point via composition engineering. This work contributes to the advancement of the field of crystal growth of high-entropy oxides. A compound with only small REs (Lu,Y,Ho,Yb,Er)2O3 maintains a cubic C-type structure upon cooling from the melt, as observed via in-situ high-temperature neutron diffraction on aerodynamically levitated samples. On the other hand, a compound with a mixture of small and large REs (Lu,Y,Ho,Nd,La)2O3 crystallizes as a mixture of a primary C-type phase with an unstable secondary phase. Crystals of compositions (Lu,Y,Ho,Nd,La)2O3 and (Lu,Y,Gd,Nd,La)2O3 were grown by the micro-pulling-down (mPD) method with a single monoclinic B-type phase, while a powder of (Lu,Y,Ho,Yb,Er)2O3 did not melt at the maximum operating temperature of an iridium-rhenium crucible. The minimization of the melting point of the two grown crystals is attributed to the mismatch in cation sizes. The electron probe microanalysis reveals that the general element segregation behavior in the crystals depends on the composition.https://doi.org/10.1007/s40145-022-0625-zhigh-entropy oxidescrystallographyneutron diffractioncrystal growth
spellingShingle Matheus Pianassola
Kaden L. Anderson
Joshua Safin
Can Agca
Jake W. McMurray
Bryan C. Chakoumakos
Jöerg C. Neuefeind
Charles L. Melcher
Mariya Zhuravleva
Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt
Journal of Advanced Ceramics
high-entropy oxides
crystallography
neutron diffraction
crystal growth
title Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt
title_full Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt
title_fullStr Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt
title_full_unstemmed Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt
title_short Tuning the melting point and phase stability of rare-earth oxides to facilitate their crystal growth from the melt
title_sort tuning the melting point and phase stability of rare earth oxides to facilitate their crystal growth from the melt
topic high-entropy oxides
crystallography
neutron diffraction
crystal growth
url https://doi.org/10.1007/s40145-022-0625-z
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