Partially collapsed cristobalite structure in the non molecular phase V in CO2.

Proc Natl Acad Sci U S A

Istituto di Fisica Applicata Nello Carrara del Consiglio Nazionale delle Ricerche (IFAC-CNR), Sesto Fiorentino, 50019 Firenze, Italy.

Published: April 2012

AI Article Synopsis

  • Non-molecular CO(2) has gained significant attention in high pressure physics and chemistry, with multiple non-molecular phases identified above 30 GPa.
  • The CO(2)-V phase resembles silica (SiO(2)) and has a structure related to β-cristobalite, although previous experimental findings had conflicting reports.
  • Recent research using advanced techniques confirmed the structure of CO(2)-V as a partially collapsed form of SiO(2) β-cristobalite, revealing important details about carbon chemistry and its implications for Earth and planetary formations.

Article Abstract

Non molecular CO(2) 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 CO(2) includes several non molecular phases above 30 GPa. Among these, the first discovered was CO(2)-V which appeared silica-like. Theoretical studies suggested that the structure of CO(2)-V is related to that of β-cristobalite with tetrahedral carbon coordination similar to silicon in SiO(2), but reported experimental structural studies have been controversial. We have investigated CO(2)-V obtained from molecular CO(2) 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 SiO(2) β-cristobalite, space group I42d, in which the CO(4) tetrahedra are tilted by 38.4° about the c-axis. The existence of CO(4) 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 SiO(2) and potential implications for Earth and planetary interiors.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC3325671PMC
http://dx.doi.org/10.1073/pnas.1118791109DOI Listing

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