Comparison of the high-pressure behavior of the cerium oxides Ce2O3 and CeO2

M. J. Lipp, J. R. Jeffries, H. Cynn, J.-H. Park Klepeis, W. J. Evans, D. R. Mortensen, G. T. Seidler, Y. Xiao, and P. Chow
Phys. Rev. B 93, 064106 – Published 9 February 2016

Abstract

The high-pressure behavior of Ce2O3 was studied using angle-dispersive x-ray diffraction to 70 GPa and compared with that of CeO2. Up to the highest pressure Ce2O3 remains in the hexagonal phase (space group 164, P3¯2/m1) typical for the lanthanide sesquioxides. A theoretically predicted phase instability for 30 GPa is not observed. The isothermal bulk modulus and its pressure derivative for the quasihydrostatic case are B0=111±2GPa,B0=4.7±0.3, and for the case without pressure-transmitting medium B0=104±4GPa,B0=6.5±0.4. Starting from ambient-pressure magnetic susceptibility measurements for both oxides in highly purified form, we find that the Ce atom in Ce2O3 behaves like a trivalent Ce3+ ion (2.57μB per Ce atom) in contrast to previously published data. Since x-ray emission spectroscopy of the Lγ (4d3/22p1/2) transition is sensitive to the 4f -electron occupancy, we also followed the high-pressure dependence of this line for both oxides up to 50 GPa. No change of the respective line shape was observed, indicating that the 4f-electron configuration is stable for both materials. We posit from this data that the 4f electrons do not drive the volume collapse of CeO2 from the high-symmetry, low-pressure fluorite structure to the lower-symmetry orthorhombic phase.

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  • Received 24 August 2015

DOI:https://doi.org/10.1103/PhysRevB.93.064106

©2016 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

M. J. Lipp1, J. R. Jeffries1, H. Cynn1, J.-H. Park Klepeis1, W. J. Evans1, D. R. Mortensen2, G. T. Seidler2, Y. Xiao3, and P. Chow3

  • 1Lawrence Livermore National Laboratory, Livermore, California 94550, USA
  • 2Physics Department, University of Washington, Seattle, Washington 98195-1560, USA
  • 3HPCAT, Geophysical Laboratory, Carnegie Institute of Washington, Argonne National Laboratory, Argonne, Illinois 60439, USA

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Issue

Vol. 93, Iss. 6 — 1 February 2016

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