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1 Division of Material Physics, Graduate School of Engineering Science, Osaka University, Toyonaka, Osaka 560-8531, Japan
2 Institute of Geophysics and Planetary Physics, University of California at Los Angels, Los Angeles 90024, U.S.A.
Correspondence: * E-mail: hama{at}user.center.osaka-u.ac.jp
By assuming an ideal two-component mixture of (Mg,Fe)SiO3 perovskite (MgPv) and (Mg,Fe)O magnesiowüstite (Mw), and by using a thermoelastic model for mantle minerals developed previously, we can reproduce the PREM values of density and velocities vP and vS of compressional and shear waves of the lower mantle within ±0.12%, ±0.28%, and ±0.56% except for the transition layers at the both boundaries. The molar fractions and atomic fractions of iron for MgPv and Mw were adjusted to reproduce the PREM values of
, vP, and vS above the point of z = 871 km (which is slightly inside the lower mantle) under constant-entropy condition. This depth avoids the boundary effect. The adiabatic bulk and shear moduli of the mixture are calculated by the Hashin-Shtrikman method for MgPv and Mw and then arithmetically averaged. The temperature profile was calculated assuming that the lower mantle is adiabatic and T(670 km) = 1873 K. The temperature at the top of D'' becomes 2444 K. Being added the temperature increment of 840 K over D (z = 27412891 km) estimated by Stacey and Loper (1983) to our value, the temperature at the core-mantle boundary (CMB) becomes 3284 K in agreement with T(CMB) of 3300 ± 500 °C by Brown and McQueen. The molar ratios of Fe/(Mg + Fe) and (Mg + Fe)/Si become 0.12 and 2.10. The calculated thermal expansivity,
, of the mixture under lower mantle conditions is in agreement with
of the lower mantle calculated directly from PEM data by Brown and Shankland, and Anderson. For the addition of 5 mol% of CaSiO3 perovskite to our model, the essential feature of the result is unchanged and the wt% of SiO2, MgO, FeO, and CaO become 40.7, 44.6, 11.0, and 3.7.
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