Confirming a pyrolitic lower mantle using self‐consistent pressure scales and new constraints on CaSiO₃ perovskite

Abstract

Abstract In this study, we have examined the lower mantle composition and mineralogy by modeling the density ( ρ ), bulk sound velocity ( V Φ ), and dln ρ /dln V Φ profiles of candidate lower mantle minerals using literature and new experimental equation of state (EoS) results. For CaSiO 3 perovskite, complimentary synchrotron X‐ray diffraction measurements in a laser‐heated diamond anvil cell were conducted up to 156 GPa between 1200 K and 2600 K to provide more reliable constraints on the thermal EoS parameters. These new experimental results as well as literature P‐V‐T data sets are systematically analyzed using an internally self‐consistent pressure scale. We have modeled ρ , V Φ , and dln ρ /dln V Φ profiles of the lower mantle with representative pyrolitic and chondritic compositional models in which the effect of Fe spin transition in ferropericlase is also taken into account. Our modeling results show that a pyrolitic lower mantle with an aggregate mineralogy of 75 vol % bridgmanite, 17 vol % ferropericlase, and 8 vol % CaSiO 3 perovskite produces ρ and V Φ profiles in better agreement with preliminary reference Earth model than a lower mantle with a chondritic composition. The modeled ρ , V Φ , and dln ρ /dln V Φ are mainly affected by the relative ratio of bridgmanite and ferropericlase but are not sensitive to the variation of the CaSiO 3 perovskite content. In addition, the spin crossover of Fe in ferropericlase can greatly raise the value of dln ρ /dln V Φ in the middle lower mantle, which is useful in detecting the presence of ferropericlase in the region. Based on these new mineral physical constraints and radial seismic structure, our study suggests the lower mantle is pyrolitic, which is chemically indistinguishable from the upper mantle.