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Coordinated Hard Sphere Mixture (CHaSM): A simplified model for oxide and silicate melts at mantle pressures and temperatures

Wolf, Aaron S. and Asimow, Paul D. and Stevenson, David J. (2015) Coordinated Hard Sphere Mixture (CHaSM): A simplified model for oxide and silicate melts at mantle pressures and temperatures. Geochimica et Cosmochimica Acta, 163 . pp. 40-58. ISSN 0016-7037. https://resolver.caltech.edu/CaltechAUTHORS:20150625-124954041

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Abstract

We develop a new model to understand and predict the behavior of oxide and silicate melts at extreme temperatures and pressures, including deep mantle conditions like those in the early Earth magma ocean. The Coordinated Hard Sphere Mixture (CHaSM) is based on an extension of the hard sphere mixture model, accounting for the range of coordination states available to each cation in the liquid. By utilizing approximate analytic expressions for the hard sphere model, this method is capable of predicting complex liquid structure and thermodynamics while remaining computationally efficient, requiring only minutes of calculation time on standard desktop computers. This modeling framework is applied to the MgO system, where model parameters are trained on a collection of crystal polymorphs, producing realistic predictions of coordination evolution and the equation of state of MgO melt over a wide range of pressures and temperatures. We find that the typical coordination number of the Mg cation evolves continuously upward from 5.25 at 0 GPa to 8.5 at 250 GPa. The results produced by CHaSM are evaluated by comparison with predictions from published first-principles molecular dynamics calculations, indicating that CHaSM is accurately capturing the dominant physics controlling the behavior of oxide melts at high pressure. Finally, we present a simple quantitative model to explain the universality of the increasing Grüneisen parameter trend for liquids, which directly reflects their progressive evolution toward more compact solid-like structures upon compression. This general behavior is opposite that of solid materials, and produces steep adiabatic thermal profiles for silicate melts, thus playing a crucial role in magma ocean evolution.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/j.gca.2015.04.018DOIArticle
http://www.sciencedirect.com/science/article/pii/S0016703715002240PublisherArticle
ORCID:
AuthorORCID
Asimow, Paul D.0000-0001-6025-8925
Stevenson, David J.0000-0001-9432-7159
Additional Information:© 2015 Elsevier Ltd. Received 11 August 2014, Accepted 10 April 2015, Available online 22 April 2015. Associate editor: Rajdeep Dasgupta. The authors would like to thank Becky Lange, Youxue Zhang, Jean-Phillipe Harvey, Jennifer M. Jackson, and Jonathan Stebbins for useful conversations throughout the development of this study. We also would like to thank the NSF for supporting this work through awards EAR-1119522 and 1226270, and the Turner Postdoctoral Fellowship at the University of Michigan.
Funders:
Funding AgencyGrant Number
NSFEAR-1119522
NSFEAR-1226270
University of Michigan Turner Postdoctoral FellowshipUNSPECIFIED
Record Number:CaltechAUTHORS:20150625-124954041
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150625-124954041
Official Citation:Aaron S. Wolf, Paul D. Asimow, David J. Stevenson, Coordinated Hard Sphere Mixture (CHaSM): A simplified model for oxide and silicate melts at mantle pressures and temperatures, Geochimica et Cosmochimica Acta, Volume 163, 15 August 2015, Pages 40-58, ISSN 0016-7037, http://dx.doi.org/10.1016/j.gca.2015.04.018. (http://www.sciencedirect.com/science/article/pii/S0016703715002240)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:58612
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:25 Jun 2015 21:24
Last Modified:03 Oct 2019 08:38

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