Electronic Spin transition in FeO\(_{2}\): evidence for Fe(II) with peroxide O\(_{2}^{2-}\)

The discovery of FeO\(_{2}\) containing more oxygen than hematite (Fe\(_{2}\)O\(_{3}\)) that was previously believed to be the most oxygen rich iron compounds, has important implications on the study of the deep lower mantle compositions. Compared to other iron compounds, there are limited reports o...

Full description

Saved in:
Bibliographic Details
Published inarXiv.org
Main Authors Jang, Bo Gyu, Liu, Jin, Hu, Qingyang, Haule, Kristjan, Ho-Kwang Mao, Mao, Wendy L, Duck Young Kim, Shim, Ji Hoon
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 21.09.2018
Subjects
Online AccessGet full text
ISSN2331-8422
DOI10.48550/arxiv.1809.07969

Cover

More Information
Summary:The discovery of FeO\(_{2}\) containing more oxygen than hematite (Fe\(_{2}\)O\(_{3}\)) that was previously believed to be the most oxygen rich iron compounds, has important implications on the study of the deep lower mantle compositions. Compared to other iron compounds, there are limited reports on FeO\(_{2}\) making studies of its physical properties of great interest in fundamental condensed matter physics and geoscience. Even the oxidation state of Fe in FeO\(_{2}\) is the subject of debate in theoretical works and there have not been reports from experimental electronic and magnetic properties measurements. Here, we report the pressure-induced spin state transition from synchrotron experiments and our computational results explain the underlying mechanism. Using density functional theory and dynamical mean field theory, we calculated spin states of Fe with volume and Hubbard interaction \(U\) change, which clearly demonstrate that Fe in FeO\(_{2}\) consists of Fe(II) and peroxide O\(_{2}^{2-}\). Our study suggests that localized nature of both Fe 3\(d\) orbitals and O\(_{2}\) molecular orbitals should be correctly treated for unveiling the structural and electronic properties of FeO\(_{2}\).
Bibliography:SourceType-Working Papers-1
ObjectType-Working Paper/Pre-Print-1
content type line 50
ISSN:2331-8422
DOI:10.48550/arxiv.1809.07969