Equations of State of Solid CO2 Phases at Megabar Pressures

2024

Closed access Metadata (CSL-JSON)
DOI 10.1134/s0021364023604165
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

The stability of CO2 phases at pressures up to 1600 GPa is confirmed using evolution methods for predicting crystal structures. Stable CO2 phases are as follows: $$I\bar {4}2d$$ (to 279 GPa), $$P{{4}_{2}}{\text{/}}nmc$$ (279–952 GPa), Pbcn (952–1018 GPa), and $$Pa\bar {3}$$ (above 1018 GPa). The equations of state for stable CO2 phases up to pressures of about 1600 GPa are calculated for the first time using ab initio methods and high-temperature calculations within the quasi-harmonic approximation. It is shown that high-pressure $$P{{4}_{2}}{\text{/}}nmc$$ , $$Pbcn$$ , and $$Pa\bar {3}$$ phases have rather high bulk moduli (290–415 GPa). Phases with sixfold coordination of carbon atoms (Pbcn and $$Pa\bar {3}$$ ) have higher coefficients of thermal expansion in comparison with the $$P{{4}_{2}}{\text{/}}nmc$$ phase.