Structure and Freezing of MgSiO 3 Liquid in Earth's Lower Mantle

Author:

Stixrude Lars12,Karki Bijaya12

Affiliation:

1. Department of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA.

2. Department of Computer Science, Louisiana State University, Baton Rouge, LA 70803, USA.

Abstract

First-principles molecular-dynamics simulations show that over the pressure regime of Earth's mantle the mean silicon-oxygen coordination number of magnesium metasilicate liquid changes nearly linearly from 4 to 6. The density contrast between liquid and crystal decreases by a factor of nearly 5 over the mantle pressure regime and is 4% at the core-mantle boundary. The ab initio melting curve, obtained by integration of the Clausius-Clapeyron equation, yields a melting temperature at the core-mantle boundary of 5400 ± 600 kelvins.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference41 articles.

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4. We use ultrasoft pseudopotentials ( 30 ) and the Vienna ab initio simulation package code which is efficient and widely tested on silicates and oxides ( 31 ). We compute the electronic structure at the Brillouin zone center and use an energy cutoff of 400 eV: Pulay (finite basis set) corrections to the pressure are found to vary linearly with V from 2 GPa at V = V X to 5 GPa at V = V X /2. To account for the error inherent in the approximation to the exchange-correlation functional we follow previous work ( 32 33 ) by adding a uniform correction of 2 GPa to the pressure in addition to the Pulay correction. The simulations are confined to the Born-Oppenheimer surface and include the influence of finite temperature on the electronic structure through the Mermin functional ( 34 ).

5. S. Nose, J. Chem. Phys.81, 511 (1984).

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