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Licensed Unlicensed Requires Authentication Published by De Gruyter June 3, 2016

High-pressure behavior of the polymorphs of FeOOH

  • Mary M. Reagan EMAIL logo , Arianna E. Gleason , Luke Daemen , Yuming Xiao and Wendy L. Mao
From the journal American Mineralogist

Abstract

The high-pressure structural and electronic behavior of α-, β-, and g-FeOOH were studied in situ using a combination of synchrotron X ray diffraction (XRD) and X ray emission spectroscopy (XES). We monitored α-FeOOH by XES as a function of pressure up to 85 GPa and observed an electronic spin transition that began at approximately 50 GPa, which is consistent with previous results. In the γ-FeOOH sample, we see the initiation of a spin transition at 35 GPa that remains incomplete up to 65 GPa. β-FeOOH does not show any indication of a spin transition up to 65 GPa. Analysis of the high-pressure XRD data shows that neither β-FeOOH nor γ-FeOOH transform to new crystal structures, and both amorphize above 20 GPa. Comparing our EOS results for the b and g phases with recently published data on the a and e phases, we found that β-FeOOH exhibits distinct behavior from the other three polymorphs, as it is significantly less compressible and does not undergo a spin transition. A systematic examination of these iron hydroxide polymorphs as a function of pressure can provide insight into the relationship between electronic spin transitions and structural transitions in these OH- and Fe3+-bearing phases that may have implications on our understanding of the water content and oxidation state of the mantle.

Acknowledgments

M.M. Reagan, A.E. Gleason, and W.L. Mao are supported by the NSF Geophysics Program (EAR-1446969). We thank Paul Chow (APS), Alastair MacDowell (ALS), and Jinyuan Yan (ALS) for their assistance with the synchrotron experiments, and Jinfu Shu (Geophysical Lab) for help with sample loading. Portions of this work were performed at beamline 12.2.2 of ALS, LBNL. ALS is supported by the Director, Office of Science, Office of Basic Energy Sciences (BES), of the U.S. Department of Energy (DOE) under Contract No. DE-AC02-05CH11231. Portions of this work were also performed at HPCAT (Sector 16), APS, ANL. HPCAT operations are supported by DOE-NNSA under Award No. DE-NA0001974 and DOE-BES under Award No. DE-FG02-99ER45775, with partial instrumentation funding by NSF. APS is a DOE-BES User Facility operated for the DOE Office of Science by ANL under Contract No. DE-AC02-06CH11357.

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Received: 2015-6-5
Accepted: 2016-2-16
Published Online: 2016-6-3
Published in Print: 2016-6-1

© 2016 by Walter de Gruyter Berlin/Boston

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