skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Determination of the high-pressure crystal structure of BaWO{sub 4} and PbWO{sub 4}

Journal Article · · Physical Review. B, Condensed Matter and Materials Physics
; ; ;  [1];  [2]; ;  [3]; ; ; ; ;  [4];  [5]
  1. Departamento Fisica Aplicada-ICMUV, Universitat de Valencia, Edificio de Investigacion, C/Dr. Moliner 50, 46100 Burjassot (Valencia) (Spain)
  2. Departamento Fisica Aplicada, Universitat Politecnica de Valencia, Camino de Vera s/n, 46022 Valencia (Spain)
  3. High Pressure Science and Engineering Center, Department of Physics, University of Nevada, 4505 Maryland Parkway, Las Vegas, Nevada 89154-4002 (United States)
  4. Departamento Fisica Fundamental II, Universidad de La Laguna, La Laguna, Tenerife (Spain)
  5. European Synchrotron Radiation Facility, BP 220, Grenoble, F-38043 (France)

We report the results of both angle-dispersive x-ray diffraction and x-ray absorption near-edge structure studies in BaWO{sub 4} and PbWO{sub 4} at pressures of up to 56 GPa and 24 GPa, respectively. BaWO{sub 4} is found to undergo a pressure-driven phase transition at 7.1 GPa from the tetragonal scheelite structure (which is stable under normal conditions) to the monoclinic fergusonite structure whereas the same transition takes place in PbWO{sub 4} at 9 GPa. We observe a second transition to another monoclinic structure which we identify as that of the isostructural phases BaWO{sub 4}-II and PbWO{sub 4}-III (space group P2{sub 1}/n). We have also performed ab initio total-energy calculations which support the stability of this structure at high pressures in both compounds. The theoretical calculations further find that upon increase of pressure the scheelite phases become locally unstable and transform displacively into the fergusonite structure. The fergusonite structure is, however, metastable and can only occur if the transition to the P2{sub 1}/n phases were kinetically inhibited. Our experiments in BaWO{sub 4} indicate that it becomes amorphous beyond 47 GPa.

OSTI ID:
20853242
Journal Information:
Physical Review. B, Condensed Matter and Materials Physics, Vol. 73, Issue 22; Other Information: DOI: 10.1103/PhysRevB.73.224103; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 1098-0121
Country of Publication:
United States
Language:
English