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1 Geosciences Department, 255 Earth and Space Sciences Building, Stony Brook University, Stony Brook, New York 11794-2100, U.S.A.
2 X-ray Science Division, Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, U.S.A.
3 GeoSoil and EnviroCARS (GSECARS), Sector 13, Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, U.S.A.
4 Chemistry Department, Stony Brook University, Stony Brook, New York 11794-3400, U.S.A.
Correspondence: * E-mail: chmartin{at}ic.sunysb.edu
Analysis of pressure-temperature dependent monochromatic X-ray powder diffraction data yield the bulk modulus [KT = 180.2(28) GPa] and thermal expansion coefficients [
0 = 2.841(34) x 105 K1;
1 = 3.37(48) x 109 K2] of CaIrO3, the structure model for post-perovskite MgSiO3. CaIrO3 is orthorhombic (Cmcm, space group 63, Z = 4) with best-fit unit-cell parameters, a = 3.14147(5) Å, b = 9.87515(19), c = 7.29711(11), and V = 226.3754(78) Å3 at 1 bar and 300 K. The c-axis of CaIrO3 has a small compressibility and a large thermal expansion when compared to the other principal axes. Rietveld structure refinement reveals changes in CaIrO3 as a function of temperature in terms of IrO6 octahedra distortion. Dissociation of CaIrO3 at high temperature has possible implications for the post-perovskite MgSiO3 structure, Earths lower mantle, and D layer.
Key Words: Post-perovskite CaIrO3 pressure temperature structure X-rays Rietveld refinement D'' layer
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C. D. Martin, R. I. Smith, W. G. Marshall, and J. B. Parise High-pressure structure and bonding in CaIrO3: The structure model of MgSiO3 post-perovskite investigated with time-of-flight neutron powder diffraction American Mineralogist, November 1, 2007; 92(11-12): 1912 - 1918. [Abstract] [Full Text] [PDF] |
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