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Structural and electron spin state changes in an x-ray heated iron carbonate system at the Earth's lower mantle pressures

Authors :
Johannes M. Kaa
Christian Sternemann
Karen Appel
Valerio Cerantola
Thomas R. Preston
Christian Albers
Mirko Elbers
Lélia Libon
Mikako Makita
Alexander Pelka
Sylvain Petitgirard
Christian Plückthun
Vladimir Roddatis
Christoph J. Sahle
Georg Spiekermann
Christian Schmidt
Anja Schreiber
Robin Sakrowski
Metin Tolan
Max Wilke
Ulf Zastrau
Zuzana Konôpková
Source :
Physical Review Research, Vol 4, Iss 3, p 033042 (2022)
Publication Year :
2022
Publisher :
American Physical Society, 2022.

Abstract

The determination of the spin state of iron-bearing compounds at high pressure and temperature is crucial for our understanding of chemical and physical properties of the deep Earth. Studies on the relationship between the coordination of iron and its electronic spin structure in iron-bearing oxides, silicates, carbonates, iron alloys, and other minerals found in the Earth's mantle and core are scarce because of the technical challenges to simultaneously probe the sample at high pressures and temperatures. We used the unique properties of a pulsed and highly brilliant x-ray free electron laser (XFEL) beam at the High Energy Density (HED) instrument of the European XFEL to x-ray heat and probe samples contained in a diamond anvil cell. We heated and probed with the same x-ray pulse train and simultaneously measured x-ray emission and x-ray diffraction of an FeCO_{3} sample at a pressure of 51 GPa with up to melting temperatures. We collected spin state sensitive Fe Kβ_{1,3} fluorescence spectra and detected the sample's structural changes via diffraction, observing the inverse volume collapse across the spin transition. During x-ray heating, the carbonate transforms into orthorhombic Fe_{4}C_{3}O_{12} and iron oxides. Incipient melting was also observed. This approach to collect information about the electronic state and structural changes from samples contained in a diamond anvil cell at melting temperatures and above will considerably improve our understanding of the structure and dynamics of planetary and exoplanetary interiors.

Subjects

Subjects :
Physics
QC1-999

Details

Language :
English
ISSN :
26431564
Volume :
4
Issue :
3
Database :
Directory of Open Access Journals
Journal :
Physical Review Research
Publication Type :
Academic Journal
Accession number :
edsdoj.124778482b2146ca923747c86b8d4890
Document Type :
article
Full Text :
https://doi.org/10.1103/PhysRevResearch.4.033042