Thermoelastic properties of MgSiO3 perovskite using the Debye approach

被引:0
|
作者
Anderson, OL [1 ]
机构
[1] Univ Calif Los Angeles, Dept Earth & Space Sci, Inst Geophys & Planetary Phys, Ctr Phys & Chem Planets, Los Angeles, CA 90095 USA
关键词
D O I
暂无
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
MgSiO3 perovskite is shown to be a Debye-like mineral by the determination of specific heat, C-V, entropy, S, and thermal pressure, Delta P-Th, using the Debye theory up to 1800 K. Sound velocities and bulk moduli at ambient conditions published by Yeganeh-Haeri were used to find the ambient acoustic Debye temperature, Theta(D)(ac). The variation of Theta(D)(ac) with T was assumed to be a curve parallel to the Theta(D)(ac) vs. T curves previously found for Al2O3, MgO, and MgSiO3, enabling Theta(D)(ac)(T) to be given up to 1800 K. To determine C-P, the thermal expansivity, alpha, and the isothermal bulk modulus, K-T, are needed. After considering several sets of alpha(T), the alpha(T) data of Funamori and his colleagues were chosen. Using the ambient K-T and the values of (partial derivative K-T/partial derivative T)(P) vs. T reported by Jackson and Rigden, K-T(T) up to 1800 K was found. Then C-P(T) up to 1800 K was found assuming quasiharmonicity in C-V. The data behind the C-P(T) calculation are also sufficient to find the Gruneisen parameter, gamma(T), and the Anderson-Gruneisen parameters, delta(T) and delta(S), up to 1800 K. The value of q = (partial derivative ln gamma/partial derivative ln V)(T) was found, and with gamma and rho, Delta P-Th vs. V and T was determined. The three sound velocities, nu(s), nu(p), and nu(b) = root K-s/rho, were then determined to 1800 K. From nu(s) and nu(p), Poisson's ratio and the isotropic shear modulus, G, were found to 1800 K. MgSiO3 perovskite is one of a small, select group of Debye-like minerals for which thermoelastic properties and the equation of state (EOS) are calculable from acoustic data.
引用
收藏
页码:23 / 35
页数:13
相关论文
共 50 条
  • [31] The mechanism of solution of aluminum oxide in MgSiO3 perovskite
    Stebbins, JF
    Kroeker, S
    Andrault, D
    GEOPHYSICAL RESEARCH LETTERS, 2001, 28 (04) : 615 - 618
  • [32] ELASTICITY OF MGSIO3 PEROVSKITE AND CHEMISTRY OF THE LOWER MANTLE
    WEIDNER, DJ
    YEGANEHHAERI, A
    CHEMICAL GEOLOGY, 1988, 70 (1-2) : 64 - 64
  • [33] Thermodynamic properties of perovskite MgSiO3 with cubic structure under extreme conditions
    Nguyen, Quang Hoc
    Ngo, Nhi Quynh
    Dao, Thi Mai
    Tran, Cong Vien
    Lai, Thi Thu Tra
    Le, Thi Van Anh
    Nguyen, Thi Thuy An
    EUROPEAN PHYSICAL JOURNAL B, 2024, 97 (10):
  • [34] MgSiO3 Post-perovskite at D" Conditions
    Wentzcovitch, Renata M.
    Tsuchiya, Taku
    Tsuchiya, Jun
    ACTA CRYSTALLOGRAPHICA A-FOUNDATION AND ADVANCES, 2005, 61 : C55 - C55
  • [35] Analysis of compressibility and thermal expansivity for MgSiO3 perovskite
    Meenakshi, S
    Sharma, BS
    INDIAN JOURNAL OF PURE & APPLIED PHYSICS, 1999, 37 (11) : 818 - 822
  • [36] COMPUTATIONAL MODEL OF THE STRUCTURAL AND ELASTIC PROPERTIES OF THE ILMENITE AND PEROVSKITE PHASES OF MGSIO3
    MATSUI, M
    AKAOGI, M
    MATSUMOTO, T
    PHYSICS AND CHEMISTRY OF MINERALS, 1987, 14 (02) : 101 - 106
  • [37] Atomistic potentials for MgSiO3 with the orthorhombic perovskite structure
    Stuart, JA
    Price, GD
    PHILOSOPHICAL MAGAZINE B-PHYSICS OF CONDENSED MATTER STATISTICAL MECHANICS ELECTRONIC OPTICAL AND MAGNETIC PROPERTIES, 1996, 73 (01): : 41 - 48
  • [38] ISOTHERMAL COMPRESSION OF PEROVSKITE-TYPE MGSIO3
    YAGI, T
    MAO, HK
    BELL, PM
    TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1978, 59 (04): : 373 - 373
  • [39] Reinvestigation of the MgSiO3 perovskite structure at high pressure
    Sugahara, M
    Yoshiasa, A
    Komatsu, Y
    Yamanaka, T
    Bolfan-Casanova, N
    Nakatsuka, A
    Sasaki, S
    Tanaka, M
    AMERICAN MINERALOGIST, 2006, 91 (04) : 533 - 536
  • [40] Sound velocity of MgSiO3 perovskite to Mbar pressure
    Murakami, Motohiko
    Sinogeikin, Stanislav V.
    Hellwig, Holger
    Bass, Jay D.
    Li, Jie
    EARTH AND PLANETARY SCIENCE LETTERS, 2007, 256 (1-2) : 47 - 54