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      Candy Wrapper for the Earth's Inner Core

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          Abstract

          Recent global expansion of seismic data motivated a number of seismological studies of the Earth's inner core that proposed the existence of increasingly complex structure and anisotropy. In the meantime, new hypotheses of dynamic mechanisms have been put forward to interpret seismological results. Here, the nature of hemispherical dichotomy and anisotropy is re-investigated by bridging the observations of PKP(bc-df) differential travel-times with the iron bcc/ hcp elastic properties computed from first-principles methods.The Candy Wrapper velocity model introduced here accounts for a dynamic picture of the inner core (i.e., the eastward drift of material), where different iron crystal shapes can be stabilized at the two hemispheres. We show that seismological data are best explained by a rather complicated, mosaic-like, structure of the inner core, where well-separated patches of different iron crystals compose the anisotropic western hemispherical region, and a conglomerate of almost indistinguishable iron phases builds-up the weakly anisotropic eastern side.

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

          A first principles theoretical approach shows that, at the density of the inner core, both hexagonal [hexagonal close-packed (hcp)] and cubic [face-centered-cubic (fcc)] phases of iron are substantially elastically anisotropic. A forward model of the inner core based on the predicted elastic constants and the assumption that the inner core consists of a nearly perfectly aligned aggregate of hcp crystals shows good agreement with seismic travel time anomalies that have been attributed to inner core anisotropy. A cylindrically averaged aggregate of fcc crystals disagrees with the seismic observations.
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            Lopsided growth of Earth's inner core.

            Hemispherical asymmetry is a prominent feature of Earth's inner core, but how this asymmetry relates to core growth is unknown. Based on multiple-scattering modeling of seismic velocity and attenuation measurements sampling the whole uppermost inner core, we propose that the growth of the solid core implies an eastward drift of the material, driven by crystallization in the Western Hemisphere and melting in the Eastern Hemisphere. This self-sustained translational motion generates an asymmetric distribution of sizes of iron crystals, which grow during their translation. The invoked dynamical process is still active today, which supports the idea of a young inner core.
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              Stability of the body-centred-cubic phase of iron in the Earth's inner core.

              Iron is thought to be the main constituent of the Earth's core, and considerable efforts have therefore been made to understand its properties at high pressure and temperature. While these efforts have expanded our knowledge of the iron phase diagram, there remain some significant inconsistencies, the most notable being the difference between the 'low' and 'high' melting curves. Here we report the results of molecular dynamics simulations of iron based on embedded atom models fitted to the results of two implementations of density functional theory. We tested two model approximations and found that both point to the stability of the body-centred-cubic (b.c.c.) iron phase at high temperature and pressure. Our calculated melting curve is in agreement with the 'high' melting curve, but our calculated phase boundary between the hexagonal close packed (h.c.p.) and b.c.c. iron phases is in good agreement with the 'low' melting curve. We suggest that the h.c.p.-b.c.c. transition was previously misinterpreted as a melting transition, similar to the case of xenon, and that the b.c.c. phase of iron is the stable phase in the Earth's inner core.
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                Author and article information

                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group
                2045-2322
                28 June 2013
                2013
                : 3
                : 2096
                Affiliations
                [1 ]Departamento de Física de la Tierra, Astronomía y Astrofísica I, Universidad Complutense de Madrid , E-28040 Madrid, Spain
                [2 ]Instituto de Geociencias (UCM-CSIC), Facultad de Ciencias Físicas , Plaza de Ciencias 1, 28040-Madrid, Spain
                [3 ]Condensed Matter Theory, Department of Theoretical Physics, AlbaNova University Center, KTH Royal Institute of Technology , SE-10691 Stockholm, Sweden
                [4 ]Research School of Earth Sciences, The Australian National University , Canberra, 0200 ACT, Australia
                [5 ]Condensed Matter Theory Group, Department of Physics and Astronomy, Uppsala University , Box 516, 75120 Uppsala, Sweden
                [6 ]Applied Materials Physics, Department of Materials Science and Engineering, Royal Institute of Technology , SE-10044 Stockholm, Sweden
                Author notes
                Article
                srep02096
                10.1038/srep02096
                3700439
                23807093
                9a9a30a3-8cd3-48f5-bf8e-2ecc6b88c1db
                Copyright © 2013, Macmillan Publishers Limited. All rights reserved

                This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit http://creativecommons.org/licenses /by/3.0/

                History
                : 18 February 2013
                : 13 June 2013
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