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JOURNALS // Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki // Archive

Pis'ma v Zh. Èksper. Teoret. Fiz., 2024 Volume 119, Issue 3, Pages 206–211 (Mi jetpl7148)

This article is cited in 1 paper

CONDENSED MATTER

Equations of state of solid CO$_2$ phases at megabar pressures

K. D. Litasova, V. V. Brazhkina, N. E. Sagatovab, T. M. Inerbaevca

a Vereshchagin Institute for High Pressure Physics, Russian Academy of Sciences, Troitsk, Moscow, 108840 Russia
b Novosibirsk State University, Novosibirsk, 630090 Russia
c Gumilyov Eurasian National University, Astana, 010008 Kazakhstan

Abstract: The stability of CO$_2$ phases at pressures up to $1600$ GPa is confirmed using evolution methods for predicting crystal structures. Stable CO$_2$ phases are as follows: $I\bar {4}2d$ (to $279$ GPa), $P4_2/nmc$ ($279$$952$ GPa), $Pbcn$ ($952$$1018$ GPa), and $Pa\bar {3}$ (above $1018$ GPa). The equations of state for stable CO$_2$ 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 $P{{4}_{2}}/nmc$, $Pbcn$, 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 $P{{4}_{2}}/nmc$ phase.

Received: 30.11.2023
Revised: 21.12.2023
Accepted: 22.12.2023

DOI: 10.31857/S123456782403008X


 English version:
Journal of Experimental and Theoretical Physics Letters, 2024, 119:3, 205–210


© Steklov Math. Inst. of RAS, 2025