High-Pressure Elasticity of Iron and Anisotropy of Earth's Inner Core

Science ◽  
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pp. 1972-1975 ◽  
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R. E. Cohen
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Daniele Antonangeli ◽  
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...  

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Florent Occelli

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...  

Eos ◽  
2020 ◽  
Vol 101 ◽  
Author(s):  
Jenessa Duncombe

How old is Earth’s inner core? High-pressure and high-temperature experiments suggest that our planet’s inner furnace may be much younger than expected.


2017 ◽  
Vol 60 (10) ◽  
pp. 1025-1032 ◽  
Author(s):  
Z G Bazhanova ◽  
V V Roizen ◽  
A R Oganov

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Matthew C. Brennan ◽  
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Samantha Couper ◽  
Lowell Miyagi ◽  
Daniele Antonangeli ◽  
...  

2019 ◽  
Vol 43 (44) ◽  
pp. 17403-17407
Author(s):  
Pengyue Gao ◽  
Chuanxun Su ◽  
Sen Shao ◽  
Sheng Wang ◽  
Peng Liu ◽  
...  

A dynamically and thermodynamically stable Fe-rich compound, Fe2Mg, reveals that Mg may be a light element candidate in the earth's inner core.


2012 ◽  
Vol 45 (2) ◽  
pp. 186-196 ◽  
Author(s):  
Lidunka Vočadlo ◽  
Ian G. Wood ◽  
David P. Dobson

First-principles calculations have been used to determine the equation of state and structural properties of NiSi up to pressures equivalent to that in the Earth's inner core. At atmospheric pressure, the thermodynamically stable phase is that with the MnP structure (as found experimentally). At high pressures, NiSi shows phase transformations to a number of high-pressure polymorphs. For pressures greater than ∼250 GPa, the thermodynamically stable phase of NiSi is that with the CsCl structure, which persists to the highest pressures simulated (∼500 GPa). At the pressures of the Earth's inner core, therefore, NiSi and FeSi will be isostructural and thus are likely to form a solid solution. The density contrast between NiSi and FeSi at inner-core pressures is ∼6%, with NiSi being the denser phase. Therefore, if a CsCl-structured (Fe,Ni)Si alloy were present in the inner core, its density (for the commonly assumed nickel content) might be expected to be ∼1% greater than that of pure FeSi.


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