SYNTHESIS AND REINVESTIGATION OF THE ELASTIC PROPERTIES OF SINGLE-CRYSTAL MAGNESIUM-SILICATE PEROVSKITE

被引:111
作者
YEGANEHHAERI, A
机构
[1] SUNY STONY BROOK,CTR HIGH PRESSURE RES,STONY BROOK,NY 11794
[2] SUNY STONY BROOK,DEPT EARTH & SPACE SCI,STONY BROOK,NY 11794
基金
美国国家科学基金会;
关键词
D O I
10.1016/0031-9201(94)90025-6
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Single crystals of MgSiO3 in the perovskite structure have been grown at a peak pressure of 26 GPa and temperature of approximately 1600 K using a 2000 ton uniaxial split-sphere high-pressure apparatus (USSA-2000). The specimens were subsequently utilized to re-investigate the single-crystal elastic properties of this phase at ambient conditions using laser Brillouin spectroscopy. The nine adiabatic single-crystal elastic stiffness coefficients, in units of GPa, are: C-11 = 482, C22 = 537, C33 = 485, C44 = 204, C55 = 186, C66 = 147, C-12 = 144, C-13 = 147, C23 = 146. The resulting estimated Voigt-Reuss-Hill (VRH) aggregate isotropic elastic moduli are: K = 264.0 and mu = 177.3 GPa, respectively. The single-crystal elastic moduli of MgSiO3 perovskite display a pattern that is elastically somewhat anisotropic. The maximum shear and compressional velocities are 18% and 7% greater than the minimum. The [010] crystallographic direction contains both the fastest and the slowest shear wave velocities. If, under lower mantle conditions, magnesium silicate perovskite grains were to become preferentially oriented, a shear wave propagating in the Earth's lower mantle could become polarized with two distinct velocities. The observed density and seismic parameter of the lower mantle over the depth range of 1000-2700 km are compared with the calculated profiles for a model mantle consisting of pure perovskite (Mg0.89,Fe0.11)SiO3 and for a mixture composed of silicate perovskite and magnesiowustite using our new elasticity results. At present, literature values of thermoelastic properties for silicate perovskite, in particular, the coefficient of thermal expansion and the temperature derivative of the isothermal bulk modulus, vary widely. Because of this disparity, we find that mantle models ranging from pure perovskite to 'pyrolitic'-type compositions provide acceptable fits to the seismically observed density and velocity profiles of the Earth's lower mantle.
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页码:111 / 121
页数:11
相关论文
共 27 条
[1]  
ANDERSON BL, 1989, THEORY EARTH
[2]   THERMODYNAMICALLY CONSISTENT DECOMPRESSION - IMPLICATIONS FOR LOWER MANTLE COMPOSITION [J].
BUKOWINSKI, MST ;
WOLF, GH .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1990, 95 (B8) :12583-12593
[3]  
DZIEWONSKI A, 1981, EARTH PLANET INTER, V15, P297
[4]  
FEI YW, 1992, PHYS CHEM MINER, V18, P416
[5]   HIGH-PRESSURE AND HIGH-TEMPERATURE INSITU X-RAY-OBSERVATION OF MGSIO3 PEROVSKITE UNDER LOWER MANTLE CONDITIONS [J].
FUNAMORI, N ;
YAGI, T .
GEOPHYSICAL RESEARCH LETTERS, 1993, 20 (05) :387-390
[7]  
HEMLEY RJ, 1992, ANNU REV EARTH PL SC, V20, P553
[8]  
HORIUCHI H, 1987, AM MINERAL, V72, P357
[9]  
Ito E., 1978, Earth and Planetary Science Letters, V38, P443, DOI 10.1016/0012-821X(78)90119-X
[10]  
ITO E, 1986, GEOPHYS RES LETT, V11, P464