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Title: Ion-irradiation-induced phase transformation in rare earth sesquioxides (Dy{sub 2}O{sub 3},Er{sub 2}O{sub 3},Lu{sub 2}O{sub 3})

Journal Article · · Journal of Applied Physics
DOI:https://doi.org/10.1063/1.2184433· OSTI ID:20787973
; ; ;  [1]
  1. Department of Materials and Metallurgical Engineering, New Mexico Institute of Mining and Technology, Socorro, New Mexico 87801 (United States) and Material Science and Technology Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)

Polycrystalline pellets of cubic C-type rare earth structure (Ia3) Dy{sub 2}O{sub 3}, Er{sub 2}O{sub 3}, and Lu{sub 2}O{sub 3} were irradiated at cryogenic temperature (120 K) with 300 keV Kr{sup ++} ions to a maximum fluence of 1x10{sup 20} Kr/m{sup 2}. Irradiated specimens were examined using grazing incidence x-ray diffraction and transmission electron microscopy. Ion irradiation leads to different radiation effects in these three materials. First, Dy{sub 2}O{sub 3} begins to transform to a monoclinic B-type rare earth structure (C2/m) at a peak dose of {approx}5 displacements per atom (dpa) (corresponding to a fluence of 2x10{sup 19} Kr/m{sup 2}). This transformation is nearly complete at a peak dose of 25 dpa (a fluence of 1x10{sup 20} Kr/m{sup 2}). Er{sub 2}O{sub 3} also transforms to the B-type structure, but the transformation starts at a higher irradiation dose of about 15-20 dpa [a fluence of about (6-8)x10{sup 19} Kr/m{sup 2}]. Lu{sub 2}O{sub 3} was found to maintain the C-type structure even at the highest irradiation dose of 25 dpa (a fluence of 1x10{sup 20} Kr/m{sup 2}). No C-to-B transformation was observed in Lu{sub 2}O{sub 3}. The irradiation dose dependence of the C-to-B phase transformation observed in Dy{sub 2}O{sub 3}, Er{sub 2}O{sub 3}, and Lu{sub 2}O{sub 3} is closely related to the temperature dependence of the C-to-B phase transformation found in phase diagrams for these three materials.

OSTI ID:
20787973
Journal Information:
Journal of Applied Physics, Vol. 99, Issue 6; Other Information: DOI: 10.1063/1.2184433; (c) 2006 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0021-8979
Country of Publication:
United States
Language:
English