CALL FOR PROPOSALS:

ORGANIZERS

  • Harvey Thorleifson, Chair
    Minnesota Geological Survey
  • Carrie Jennings, Vice Chair
    Minnesota Geological Survey
  • David Bush, Technical Program Chair
    University of West Georgia
  • Jim Miller, Field Trip Chair
    University of Minnesota Duluth
  • Curtis M. Hudak, Sponsorship Chair
    Foth Infrastructure & Environment, LLC

 

Paper No. 4
Presentation Time: 9:20 AM

STRUCTURE IN DICHALCOGENIDES AT HIGH PRESSURE


ROSS, Nancy, Dept. of Geosciences, Virginia Tech, 4044 Derring Hall, Blacksburg, VA 24061 and YU, Yonggang, Institut für Geowissenschaften, Goethe-Universität, Altenhöferallee 1, Frankfurt, 60438, Germany, nross@vt.edu

The structural and vibrational properties of TiS2 with the CdI2 structure have been studied to high pressures from density functional calculations within the local density approximation (LDA). The calculated axial compressibility of the CdI2-type phase agrees well with experimental data and is typical of layered transition-metal dichalcogenides. The calculated phonon frequencies also show good correspondence with available experiments. Our LDA study predicts that the CdI2-type TiS2, the phase stable at ambient conditions, should transform to the cotunnite phase at 15.1 GPa, in good agreement with the results of Yu et al. [1]. However, we also predict a further transition from the cottunite phase to a tetragonal phase (I 4/mmm) at 45.0 GPa. The tetragonal phase has a structure similar to that of MoSi2 and consists of layers of NiS8 tetragonal prisms which share faces within the layers. The possible existence of the MoSi2 phase at high pressures is consistent with our previous findings in NiS2 [2]. In addition, recent simulations on ZrSe2, which also crystallizes with the CdI2 structure under ambient conditions, suggest that there is a direct transformation from the CdI2 structure to the MoSi2 phase at pressures less than 10 GPa.

[1] Yu F, Sun J-X, Zhou Y-H (2010) Solid State Sciences 12: 1786-1790; [2] Yu Y and Ross NL (2010) J. Phys: Cond. Matter 22:235401.

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