Solidus and liquidus profiles of chondritic mantle: Implication for melting of the Earth across its history

By D. Andrault, N. Bolfan-Casanova, G. L. Nigro, M. Bouhifd, G. Garbarino, M. Mezouar. 2011

334 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/8cadc8fedc97c1546e2cc98d6e38c4a2fb30442a

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In Geophysics

Citations in the corpus

Thermal evolution of an early magma ocean in interaction with the atmosphere (2012, neutral): “But this is still debated [ Andrault et al. , 2011].”
Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water (2014, background): “her pressures (>24 GPa). The melting temperatures of Liebske and Frost (2012) are based on a thermodynamic model; their mantle liquidus temperatures are close to those determined experimentally by Andrault et al. (2010) but at temperatures that lie are several 100 K below the liquidus temperature”
Energetics of the Core (2015, background): “This issue is discussed in more detail in Nimmo**. and liquidus temperatures for the lowermost mantle (Andrault et al. 2011); arrow indicates estimated present CMB core temperature. b) Variation in inner core age as a function of core potassium concentration and entropy production rate.”
Dynamics and evolution of the deep mantle resulting from thermal, chemical, phase and melting effects (2012, background): “, 2011), although there is still some uncertainty about this scenario (Andrault et al., 2011).”
Thermal evolution of the core with a high thermal conductivity (2014, neutral): “The initial temperature from the calculation corresponding to ﬁgure 11 (solid line) is about 7800K and is well above the liquidus of peridotite and a “chondritic” mantle, as determined by Fiquet et al. (2010) and Andrault et al. (2011), respectively.”