Electronic and magnetic structures of the postperovskite-type Fe 2O 3 and implications for planetary magnetic records and deep interiors

Proceedings of the National Academy of Sciences of the United States of America

Volumn 106, Issue 14, 2009, Pages 5508-5512

  Shim, Sang Heon ^a   Bengtson, Amelia ^b   Morgan, Dane ^b   Sturhahn, Wolfgang ^c   Catalli, Krystle ^a   Zhao, Jiyong ^c   Lerche, Michael ^c,d   Prakapenka, Vitali ^e  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b University of Wisconsin Madison   (United States)

^c ARGONNE NATIONAL LABORATORY   (United States)

^d CARNEGIE INSTITUTION OF WASHINGTON   (United States)

^e UNIVERSITY OF CHICAGO   (United States)

Author keywords

Electrical conductivity; High pressure; Phase transition; Spin ordering

Indexed keywords

FERRIC OXIDE;

ARTICLE; CHEMICAL REACTION; CRYSTAL STRUCTURE; ELECTRIC CONDUCTIVITY; MAGNETIC FIELD; MOSSBAUER SPECTROSCOPY; PRIORITY JOURNAL; SEMICONDUCTOR; SYNCHROTRON; X RAY DIFFRACTION;

ELECTRIC CONDUCTIVITY; FERRIC COMPOUNDS; MAGNETICS; MODELS, MOLECULAR; PLANETS; PRESSURE; SPECTROSCOPY, MOSSBAUER; X-RAY DIFFRACTION;

EID: 65249117008     PISSN: 00278424     EISSN: 10916490     Source Type: Journal    
DOI: 10.1073/pnas.0808549106     Document Type: Article

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