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doi:10.1016/j.pepi.2007.06.012    
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Copyright © 2007 Elsevier B.V. All rights reserved.

Ab initio calculations of the elastic properties of ferropericlase Mg1−xFexO (x≤0.25)

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L. Kočia, Corresponding Author Contact Information, E-mail The Corresponding Author, E-mail The Corresponding Author, L. Vitosa, b, c and R. Ahujaa, b

aCondensed Matter Theory Group, Physics Department, Uppsala University, Box 530, S-751 21 Uppsala, Sweden

bApplied Materials Physics, Department of Materials Science and Engineering, The Royal Institute of Technology, SE-10044 Stockholm, Sweden

cResearch Institute for Solid State Physics and Optics, P.O. Box 49, H-1525 Budapest, Hungary


Received 7 March 2007; 
revised 6 June 2007; 
accepted 29 June 2007. 
Available online 20 July 2007.

Abstract

Ferropericlase Mg1−xFexO is believed to be the second most abundant mineral in the Earth’s mantle. Therefore, the electronic and elastic properties of ferropericlase are important for the understanding of the Earth’s interior. Ab initio total energy calculations have been performed for Fe concentrations x≤0.25. The equation of state (EOS) clearly shows a volume expansion as a function of Fe concentration, consistent with experimental data. Magnetic moment calculations as a function of pressure show a high-spin to low-spin transition of Fe2+, and the theoretical transition pressure increases with iron composition. At ambient pressure, we have found that the shear constant C44 reproduces well the experimental data as a function of Fe concentration. The MgO and Mg0.9Fe0.1O minerals show an increasing C44 with pressure, whereas the View the MathML source is slightly negative after 26 GPa for Mg0.8Fe0.2O. The C44 softening could be related to the transition from the cubic to a rhombohedrally distorted phase, recently found by experiment.

Keywords: Ferropericlase; Elasticity; Pressure

Article Outline

1. Introduction
2. Theory
2.1. Methods
2.2. Equation of state
2.3. Elastic constant calculations
2.4. Numerical data
3. Results
3.1. MgO
3.2. (Mg,Fe)O
3.2.1. Magnetic structure
3.2.2. EOS and elastic constants
4. Discussion and summary
Acknowledgements
References







Corresponding Author Contact InformationCorresponding author.

 
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