Equation of state and spin crossover of (Mg,Fe)O at high pressure, with implications for explaining topographic relief at the core-mantle boundary
-
Natalia V. Solomatova
, Jennifer M. Jackson
, Wolfgang Sturhahn , June K. Wicks , Jiyong Zhao , Thomas S. Toellner , Bora Kalkan and William M. Steinhardt
Abstract
Iron-bearing periclase is thought to represent a significant fraction of Earth’s lower mantle. However, the concentration of iron in (Mg,Fe)O is not well constrained at all mantle depths. Therefore, understanding the effect of iron on the density and elastic properties of this phase plays a major role in interpreting seismically observed complexity in the deep Earth. Here we examine the high-pressure behavior of polycrystalline (Mg,Fe)O containing 48 mol% FeO, loaded hydrostatically with neon as a pressure medium. Using X-ray diffraction and synchrotron Mössbauer spectroscopy, we measure the equation of state to about 83 GPa and hyperfine parameters to 107 GPa at 300 K. A gradual volume drop corresponding to a high-spin (HS) to low-spin (LS) crossover is observed between ~45 and 83 GPa with a volume drop of 1.85% at 68.8(2.7) GPa, the calculated spin transition pressure. Using a newly formulated spin crossover equation of state, the resulting zero-pressure isothermal bulk modulus K0T,HS for the HS state is 160(2) GPa with a 

Acknowledgments
We thank E.E. Alp and W. Bi for the isomer shift measurement of the reference stainless steel foil. We are thankful to NSF-EAR-CAREER-0956166, NSF-CSEDI-EAR-1161046, and COMPRES, which partially supports operations at Sector 3 (APS), the Mössbauer Laboratory (APS), and Beamline 12.2.2 (ALS). Ambient X-ray diffraction experiments at 11-BM of APS were made possible by Saul Lapidus and Lynn Ribaud. Microprobe analyses at Caltech were partially funded by MRSEX Program of the NSF under DMR-0080065. Ruby fluorescence measurements for the SMS experiments were conducted at GSE-CARS. Use of the Advanced Photon Source is supported by the U.S. DOE, Office of Science (DE-AC02-06CH11357). The Advanced Light Source is supported by the U.S. DOE, Office of Science (DE-AC02-05CH11231). We thank two anonymous reviewers for their thoughtful comments.
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- Presidential Address
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