Elastic and attenuation anisotropy in directionally solidified (hcp) zinc, and the seismic anisotropy in the Earth's inner core

2000 ◽  
Vol 117 (1-4) ◽  
pp. 139-151 ◽  
Author(s):  
Michael I Bergman ◽  
Louis Giersch ◽  
Michael Hinczewski ◽  
Valerie Izzo
2014 ◽  
Vol 346 (5-6) ◽  
pp. 140-147 ◽  
Author(s):  
Michael I. Bergman ◽  
Yahya Al-Khatatbeh ◽  
Daniel J. Lewis ◽  
Margarita C. Shannon

Minerals ◽  
2019 ◽  
Vol 9 (12) ◽  
pp. 720
Author(s):  
Jing Yang ◽  
Yingwei Fei ◽  
Xiaojun Hu ◽  
Eran Greenberg ◽  
Vitali B. Prakapenka

Understanding the effect of carbon on the density of hcp (hexagonal-close-packed) Fe-C alloys is essential for modeling the carbon content in the Earth’s inner core. Previous studies have focused on the equations of state of iron carbides that may not be applicable to the solid inner core that may incorporate carbon as dissolved carbon in metallic iron. Carbon substitution in hcp-Fe and its effect on the density have never been experimentally studied. We investigated the compression behavior of Fe-C alloys with 0.31 and 1.37 wt % carbon, along with pure iron as a reference, by in-situ X-ray diffraction measurements up to 135 GPa for pure Fe, and 87 GPa for Fe-0.31C and 109 GPa for Fe-1.37C. The results show that the incorporation of carbon in hcp-Fe leads to the expansion of the lattice, contrary to the known effect in body-centered cubic (bcc)-Fe, suggesting a change in the substitution mechanism or local environment. The data on axial compressibility suggest that increasing carbon content could enhance seismic anisotropy in the Earth’s inner core. The new thermoelastic parameters allow us to develop a thermoelastic model to estimate the carbon content in the inner core when carbon is incorporated as dissolved carbon hcp-Fe. The required carbon contents to explain the density deficit of Earth’s inner core are 1.30 and 0.43 wt % at inner core boundary temperatures of 5000 K and 7000 K, respectively.


2013 ◽  
Vol 223 ◽  
pp. 32-39 ◽  
Author(s):  
Yahya Al-Khatatbeh ◽  
Michael I. Bergman ◽  
Daniel J. Lewis ◽  
Zachary Mason ◽  
Laura Zhu ◽  
...  

2021 ◽  
Author(s):  
Daniel Frost ◽  
Marine Lasbleis ◽  
Brian Chandler ◽  
Barbara Romanowicz

Abstract Progressive crystallisation of Earth's inner core over geological times drives convection in the outer core and the generation of the Earth’s magnetic field. Resolving the rate and pattern of inner core growth is thus crucial to understanding the evolution of the geodynamo. The growth history of Earth’s inner core is likely recorded in the distribution and strength of seismic anisotropy arising from deformation texturing constrained by boundary conditions at the inner-core solid-fluid boundary. Travel times of seismic body waves indicate that seismic anisotropy increases with depth. Here we find that the strongest anisotropy is offset from Earth's rotation axis. Using geodynamic growth models and mineral physics calculations, we simulate the development of inner core anisotropy in a self-consistent manner. We show for the first time that an inner core model composed of hexagonally close-packed iron-nickel alloy, deformed by a combination of preferential equatorial growth and slow translation can match the seismic observations without requiring the introduction of hemispheres with sharp boundaries. We find a model of the inner core growth history compatible with external constraints from outer core dynamics, supporting arguments for a relatively young inner core (~0.5-1.5 Ga) and a viscosity >1018 Pa-s.


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