Partially collapsed cristobalite structure in the non molecular phase V in CO2
Non molecular CO2 has been an important subject of study in high pressure physics and chemistry for the past decade opening up a unique area of carbon chemistry. The phase diagram of CO2 includes several non molecular phases above 30 GPa. Among these, the first discovered was CO2-V which appeared si...
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Published in | Proceedings of the National Academy of Sciences - PNAS Vol. 109; no. 14; pp. 5176 - 5179 |
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Main Authors | , , , , , , , |
Format | Journal Article |
Language | English |
Published |
United States
National Academy of Sciences
03.04.2012
National Acad Sciences |
Subjects | |
Online Access | Get full text |
ISSN | 0027-8424 1091-6490 1091-6490 |
DOI | 10.1073/pnas.1118791109 |
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Summary: | Non molecular CO2 has been an important subject of study in high pressure physics and chemistry for the past decade opening up a unique area of carbon chemistry. The phase diagram of CO2 includes several non molecular phases above 30 GPa. Among these, the first discovered was CO2-V which appeared silica-like. Theoretical studies suggested that the structure of CO2-V is related to that of β-cristobalite with tetrahedral carbon coordination similar to silicon in SiO2, but reported experimental structural studies have been controversial. We have investigated CO2-V obtained from molecular CO2 at 40–50 GPa and T > 1500 K using synchrotron X-ray diffraction, optical spectroscopy, and computer simulations. The structure refined by the Rietveld method is a partially collapsed variant of SiO2 β-cristobalite, space group Formula , in which the CO4 tetrahedra are tilted by 38.4° about the c-axis. The existence of CO4 tetrahedra (average O-C-O angle of 109.5°) is thus confirmed. The results add to the knowledge of carbon chemistry with mineral phases similar to SiO2 and potential implications for Earth and planetary interiors. |
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Bibliography: | http://dx.doi.org/10.1073/pnas.1118791109 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 PMCID: PMC3325671 Author contributions: M.S., F.A.G., and J.H. designed research; M.S., F.A.G., R.B., J.H., O.C., C.L., J.A.M., and S.S. performed research; M.S., R.B., J.H., J.A.M., and S.S. analyzed data; and M.S. and J.H. wrote the paper. Edited by Russell J. Hemley, Carnegie Institution of Washington, Washington, DC, and approved January 24, 2012 (received for review November 16, 2011) |
ISSN: | 0027-8424 1091-6490 1091-6490 |
DOI: | 10.1073/pnas.1118791109 |