TY - JOUR
T1 - First principles thermoelasticity of MgSiO3-perovskite
T2 - Consequences for the inferred properties of the lower mantle
AU - Karki, Bijaya B.
AU - Wentzcovitch, Renata M.
AU - De Gironcoli, Stefano
AU - Baroni, Stefano
PY - 2001/7/15
Y1 - 2001/7/15
N2 - Some key thermoelastic properties of MgSiO3- perovskite (pv) have been determined at lower mantle (LM) pressures and temperatures using the quasi-harmonic approximation in conjunction with first principles phonon dispersions. The adiabatic bulk moduli (KS) of pv and of an assemblage of 80 vol% pv and 20 vol% MgO were obtained along the thermodynamically inferred adiabat and compared with the seismic counterpart given by the preliminary reference Earth model (KPREM). The discrepancy between calculated KS's and KPREM in the deep LM suggests a super-adiabatic gradient, or subtle changes of composition, or phase, or all beginning at about 1200 km. The Anderson Grüneisen parameter, δs = (∂lnKs/∂lnρ)P, was predicted to decrease rapidly with a depth (from 2.7 to 1.2 across the LM) supporting the thermal origin for the lateral heterogeneities throughout most of the LM.
AB - Some key thermoelastic properties of MgSiO3- perovskite (pv) have been determined at lower mantle (LM) pressures and temperatures using the quasi-harmonic approximation in conjunction with first principles phonon dispersions. The adiabatic bulk moduli (KS) of pv and of an assemblage of 80 vol% pv and 20 vol% MgO were obtained along the thermodynamically inferred adiabat and compared with the seismic counterpart given by the preliminary reference Earth model (KPREM). The discrepancy between calculated KS's and KPREM in the deep LM suggests a super-adiabatic gradient, or subtle changes of composition, or phase, or all beginning at about 1200 km. The Anderson Grüneisen parameter, δs = (∂lnKs/∂lnρ)P, was predicted to decrease rapidly with a depth (from 2.7 to 1.2 across the LM) supporting the thermal origin for the lateral heterogeneities throughout most of the LM.
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U2 - 10.1029/2001GL012910
DO - 10.1029/2001GL012910
M3 - Article
AN - SCOPUS:0035878291
SN - 0094-8276
VL - 28
SP - 2699
EP - 2702
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 14
ER -