Stability and properties of liquid CO2 at high pressure and high temperature: Implications for electrical conductivities in Earth's lower mantle
Carbon dioxide (CO2), one of the most important planetary materials, has been the subject of extensive experimental and theoretical studies. However, the stabilities and properties of CO2 at high pressures and temperatures relevant to Earth's mantle and core remain controversial. We have studie...
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Published in | Geophysical research letters Vol. 42; no. 14; pp. 5820 - 5827 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Washington
Blackwell Publishing Ltd
28.07.2015
John Wiley & Sons, Inc |
Subjects | |
Online Access | Get full text |
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Summary: | Carbon dioxide (CO2), one of the most important planetary materials, has been the subject of extensive experimental and theoretical studies. However, the stabilities and properties of CO2 at high pressures and temperatures relevant to Earth's mantle and core remain controversial. We have studied the molten structures of CO2‐V with first‐principles molecular dynamic calculations at 60 GPa and different temperatures. The formation of oxygen molecules in the melt is consistent with experimental observations. In particular, the melting transition is accompanying by metallization. The metallic behavior is shown to originate from electron delocalization between oxygen via the overlap of the π orbitals from the dissociated oxygen‐rich species. Metallic molten CO2 is a potential candidate to explain the high conductivities of the Earth's lower mantle. Furthermore, theoretical results do not support the existence of the proposed ionic solid phase of CO2 at high temperature and high pressure.
Key Points
Dissociation of carbon dioxide at high pressure and high temperature
Metallization of carbon dioxide at high pressure and temperature
Molten CO2 may be a contributing factor to the high conductivity of the Earth's mantle |
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Bibliography: | ArticleID:GRL53152 ark:/67375/WNG-H1WLDC47-J Text S1 and Figures S1 and S2 istex:626E30D9F50A559581C762DB3EEA0DFBFBADD25B ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1002/2015GL064522 |