Solid Earth
Grüneisen parameter of hcp-Fe to 171 GPa
Article first published online: 20 DEC 2011
DOI: 10.1029/2011GL049531
Copyright 2011 by the American Geophysical Union.
Additional Information
How to Cite
, , , and (2011), Grüneisen parameter of hcp-Fe to 171 GPa, Geophys. Res. Lett., 38, L24306, doi:10.1029/2011GL049531.
Publication History
- Issue published online: 20 DEC 2011
- Article first published online: 20 DEC 2011
- Manuscript Accepted: 6 NOV 2011
- Manuscript Revised: 3 NOV 2011
- Manuscript Received: 2 SEP 2011
Keywords:
- Earth's core;
- Grüneisen parameter;
- Iron;
- high pressure;
- phonon density of states
[1] We measured the phonon density of states (DOS) of hexagonal close-packed iron (ɛ-Fe) with high statistical quality using nuclear resonant inelastic X-ray scattering and in situ X-ray diffraction experiments between pressures of 30 GPa and 171 GPa and at 300 K, with a neon pressure medium up to 69 GPa. The shape of the phonon DOS remained similar at all compression points, while the maximum (cutoff) energy increased regularly with decreasing volume. As a result, we present a generalized scaling law to describe the volume dependence of ɛ-Fe's total phonon DOS which, in turn, is directly related to the ambient temperature vibrational Grüneisen parameter (γvib). Fitting our individual γvib data points with γvib = γvib,0(V/V0)q, a common parameterization, we found an ambient pressure γvib,0 = 2.0 ± 0.1 for the range q = 0.8 to 1.2. We also determined the Debye sound velocity (vD) from the low-energy region of the phonon DOS and our in situ measured volumes, and used the volume dependence of vD to determine the commonly discussed Debye Grüneisen parameter (γD). Comparing our γvib(V) and γD(V), we found γvib to be ∼10% larger than γD at any given volume. Finally, applying our γvib(V) to a Mie-Grüneisen type relationship and an approximate form of the empirical Lindemann melting criterion, we predict the vibrational thermal pressure and estimate the high-pressure melting behavior of ɛ-Fe at Earth's core pressures.

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