The MgSiO3 system at high pressure: Thermodynamic properties of perovskite, postperovskite, and melt from global inversion of shock and static compression data

145 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Dynamics and evolution of the deep mantle resulting from thermal, chemical, phase and melting effects (2012, background): “Shock-wave experiments (Akins et al., 2004; Mosenfelder et al., 2007; Mosenfelder et al., 2009) indicate that melt may indeed be slightly denser than perovskite, although less dense than post-perovskite (Mosenfelder et al.”
Solidus and liquidus profiles of chondritic mantle: Implication for melting of the Earth across its history (2011, methodology): “Indeed the forsterite liquidus is observed to be lower than that of enstatite at high-pressures (Mosenfelder et al., 2009).”
Mantle dynamics in super-Earths: Post-perovskite rheology and self-regulation of viscosity (2012, background): “…Earth’s CMB pressure, consistent with mineral physics 299 constraints (Chopelas and Boehler, 1992; Katsura et al., 2010; Komabayashi et al., 2008; 300 Mosenfelder et al., 2009), and to about 1.5x10-6 K-1 at 1400 GPa, which appears to be 301 consistent with that estimated by (Stamenković et…”
Very low sound velocities in iron‐rich (Mg,Fe)O: Implications for the core‐mantle boundary region (2010, background): “These ultra‐low velocity zones (ULVZs) have been attributed to a metal‐bearing layer [Manga and Jeanloz, 1996], iron‐enriched post‐perovskite [Mao et al., 2004], and most popularly to partial melting [Williams et al., 1998; Lay et al., 2004; Labrosse et al., 2007; Mosenfelder et al., 2009].”