<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Morard G</submitter><funding>European Research Council</funding><pagination>e2022JB025117</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC9788056</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>127(11)</volume><pubmed_abstract>FeO represents an important end-member for planetary interiors mineralogy. However, its properties in the liquid state under high pressure are poorly constrained. Here, in situ high-pressure and high-temperature X-ray diffraction experiments, ab initio simulations, and thermodynamic calculations are combined to study the local structure and density evolution of liquid FeO under extreme conditions. Our results highlight a strong shortening of the Fe-Fe distance, particularly pronounced between ambient pressure and ∼40 GPa, possibly related with the insulator to metal transition occurring in solid FeO over a similar pressure range. Liquid density is smoothly evolving between 60 and 150 GPa from values calculated for magnetic liquid to those calculated for non-magnetic liquid, compatibly with</pubmed_abstract><journal>Journal of geophysical research. Solid earth</journal><pubmed_title>Structural and Electronic Transitions in Liquid FeO Under High Pressure.</pubmed_title><pmcid>PMC9788056</pmcid><funding_grant_id>670787</funding_grant_id><funding_grant_id>724690</funding_grant_id><pubmed_authors>Rivoldini A</pubmed_authors><pubmed_authors>Chariton S</pubmed_authors><pubmed_authors>Boulard E</pubmed_authors><pubmed_authors>Greenberg E</pubmed_authors><pubmed_authors>Morard G</pubmed_authors><pubmed_authors>Mezouar M</pubmed_authors><pubmed_authors>Antonangeli D</pubmed_authors><pubmed_authors>Prescher C</pubmed_authors><pubmed_authors>Miozzi F</pubmed_authors><pubmed_authors>Bureau H</pubmed_authors><pubmed_authors>Bouchet J</pubmed_authors><pubmed_authors>Boccato S</pubmed_authors></additional><is_claimable>false</is_claimable><name>Structural and Electronic Transitions in Liquid FeO Under High Pressure.</name><description>FeO represents an important end-member for planetary interiors mineralogy. However, its properties in the liquid state under high pressure are poorly constrained. Here, in situ high-pressure and high-temperature X-ray diffraction experiments, ab initio simulations, and thermodynamic calculations are combined to study the local structure and density evolution of liquid FeO under extreme conditions. Our results highlight a strong shortening of the Fe-Fe distance, particularly pronounced between ambient pressure and ∼40 GPa, possibly related with the insulator to metal transition occurring in solid FeO over a similar pressure range. Liquid density is smoothly evolving between 60 and 150 GPa from values calculated for magnetic liquid to those calculated for non-magnetic liquid, compatibly with</description><dates><release>2022-01-01T00:00:00Z</release><publication>2022 Nov</publication><modification>2025-04-18T22:24:45.301Z</modification><creation>2025-04-07T10:10:11.578Z</creation></dates><accession>S-EPMC9788056</accession><cross_references><pubmed>36590903</pubmed><doi>10.1029/2022JB025117</doi></cross_references></HashMap>