DI006-0017
Spin transitions and compressibility of ε-Fe7N3 and γ’-Fe4N: implications for iron alloys in terrestrial planetary cores

Wednesday, 9 December 2020
Poster
Mingda Lv1, Jiachao Liu1, Feng Zhu2, Jie Li2, Dongzhou Zhang3, Yuming Xiao4 and Susannah Dorfman1, (1)Michigan State University, Earth and Environmental Sciences, East Lansing, MI, United States, (2)University of Michigan Ann Arbor, Department of Earth and Environmental Sciences, Ann Arbor, MI, United States, (3)University of Hawaii at Manoa, Hawaii Institute of Geophysics and Planetology, School of Ocean and Earth Science and Technology, Honolulu, HI, United States, (4)Argonne National Laboratory, High Pressure Collaborative Access Team, X-ray Science Division, Argonne, IL, United States
Abstract:
Iron nitrides are possible constituents in the cores of the Earth and other terrestrial planets. Pressure-induced magnetic changes in iron nitrides and their effects on elasticity remain poorly understood. Here we report synchrotron X-ray emission spectroscopy (XES) and X-ray diffraction (XRD) data of ε-Fe7N3 and γ’-Fe4N compressed up to 60 GPa at 300 K using diamond anvil cells. The XES spectra reveal completion of high- to low-spin state transition in ε-Fe7N3 and γ’-Fe4N within the experimental pressure range. The spin transition induces elastic stiffening in ε-Fe7N3 but has no resolvable effect on the compression behavior of γ’-Fe4N. We re-examine evidence for spin transition and effects on compressibility of other candidate components of terrestrial planet cores, Fe3S, Fe3P, Fe7C3, and Fe3C based on previous XES and XRD measurements, illustrating composition dependence of the pressure and effects of high- to low-spin transition. The changes in incompressibility induced by spin transition are important for evaluating the role of light element in iron-rich cores.