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Licensed Unlicensed Requires Authentication Published by De Gruyter November 28, 2018

Electronic properties and compressional behavior of Fe–Si alloys at high pressure

  • Seiji Kamada EMAIL logo , Nanami Suzuki , Fumiya Maeda , Naohisa Hirao , Maki Hamada , Eiji Ohtani , Ryo Masuda , Takaya Mitsui , Yasuo Ohishi and Satoshi Nakano
From the journal American Mineralogist


Planetary cores are composed mainly of Fe with minor elements such as Ni, Si, O, and S. The physical properties of Fe alloys depend on their composition. Changes in c/a ratio, center shifts, and elastic properties of Fe and Fe–Ni alloys were reported previously. However, such properties of Fe light-element alloys have not yet been extensively studied. Si is a plausible candidate as a light element in planetary cores. Therefore, we studied the electronic properties and compressional behavior of Fe-Si alloys with a hexagonal-close-packed (hcp) structure under high pressure using synchrotron Mössbauer spectroscopy (SMS) and X‑ray diffraction (XRD). Center shifts (CS) were observed at pressures of 21.4–45.3 GPa for Fe-2.8wt%Si and of 30.9–62.2 GPa for Fe-6.1wt%Si. Some of SMS and XRD measurements were performed under the same conditions using a newly developed system at the BL10XU beamline of SPring-8, which allowed simultaneous characterization of the electron information and crystal structure. Changes in the CS values were observed at 36.9 GPa in Fe-2.8wt%Si and 54.3 GPa in Fe-6.1wt%Si. The ratios of c/a in the hcp structure were measured at pressures of 21.2–49.6 GPa in Fe-2.8wt%Si and 32.9–61.4 GPa in Fe-6.1wt%Si. The c/a ratio changed at pressures of 30–45 GPa in Fe-2.8wt%Si and at 50 GPa in Fe-6.1wt%Si. Changes in the CS and c/a ratio were explained according to the electronic isostructural transition in Fe–Si alloys. In addition, the transition pressure increased with increasing Si content in metallic iron. This finding is significant as changes in seismic wave velocities due to the change in c/a ratio of Fe–Si alloys with an hcp structure might be observed if Venus has a solid inner core.


S.K. was supported by a Grant-in-Aid for Young Scientists (B) (no. 25800291) and E.O. was supported by a Grant-in-Aid for Scientific Research from the Ministry of Education, Culture, Science, Sport and Technology of the Japanese Government (nos. 22000002 and 15H05748). The synchrotron radiation experiments were performed at the SPring-8 facility with the approval of the Japan Synchrotron Radiation Research Institute (proposal nos. 2013A1496, 2013A3513, 2013B0104, 2013A3517, 2014A0104, 2014A1910, 2014A3516, 2014B0104, 2014A3519, 2015A0104, and 2015B0104) and Japan Atomic Energy Agency (proposal nos. 2013A-E01, 2013B-E07, 2014A-E06, and 2014B-E09).

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Received: 2017-12-08
Accepted: 2018-08-14
Published Online: 2018-11-28
Published in Print: 2018-12-19

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