Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics

Ab initio molecular dynamics simulations were performed to investigate the elasticity of cubic CaSiO3 perovskite at high pressure and temperature. All three independent elastic constants for cubic CaSiO3 perovskite, C11, C12, and C44, were calculated from the computation of stress generated by small...

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Main Author: Shigeaki Ono
Format: Article
Language:English
Published: MDPI AG 2013-10-01
Series:Entropy
Subjects:
Online Access:http://www.mdpi.com/1099-4300/15/10/4300
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author Shigeaki Ono
author_facet Shigeaki Ono
author_sort Shigeaki Ono
collection DOAJ
description Ab initio molecular dynamics simulations were performed to investigate the elasticity of cubic CaSiO3 perovskite at high pressure and temperature. All three independent elastic constants for cubic CaSiO3 perovskite, C11, C12, and C44, were calculated from the computation of stress generated by small strains. The elastic constants were used to estimate the moduli and seismic wave velocities at the high pressure and high temperature characteristic of the Earth’s interior. The dependence of temperature for sound wave velocities decreased as the pressure increased. There was little difference between the estimated compressional sound wave velocity (VP) in cubic CaSiO3 perovskite and that in the Earth’s mantle, determined by seismological data. By contrast, a significant difference between the estimated shear sound wave velocity (VS) and that in the Earth’s mantle was confirmed. The elastic properties of cubic CaSiO3 perovskite cannot explain the properties of the Earth’s lower mantle, indicating that the cubic CaSiO3 perovskite phase is a minor mineral in the Earth’s lower mantle.
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spelling doaj.art-a17acf73adb540d8b514f01687fa00122022-12-22T02:55:41ZengMDPI AGEntropy1099-43002013-10-0115104300430910.3390/e15104300Elastic Properties of CaSiO3 Perovskite from ab initio Molecular DynamicsShigeaki OnoAb initio molecular dynamics simulations were performed to investigate the elasticity of cubic CaSiO3 perovskite at high pressure and temperature. All three independent elastic constants for cubic CaSiO3 perovskite, C11, C12, and C44, were calculated from the computation of stress generated by small strains. The elastic constants were used to estimate the moduli and seismic wave velocities at the high pressure and high temperature characteristic of the Earth’s interior. The dependence of temperature for sound wave velocities decreased as the pressure increased. There was little difference between the estimated compressional sound wave velocity (VP) in cubic CaSiO3 perovskite and that in the Earth’s mantle, determined by seismological data. By contrast, a significant difference between the estimated shear sound wave velocity (VS) and that in the Earth’s mantle was confirmed. The elastic properties of cubic CaSiO3 perovskite cannot explain the properties of the Earth’s lower mantle, indicating that the cubic CaSiO3 perovskite phase is a minor mineral in the Earth’s lower mantle.http://www.mdpi.com/1099-4300/15/10/4300perovskitefirst-principles calculationseismic wave velocity
spellingShingle Shigeaki Ono
Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics
Entropy
perovskite
first-principles calculation
seismic wave velocity
title Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics
title_full Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics
title_fullStr Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics
title_full_unstemmed Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics
title_short Elastic Properties of CaSiO3 Perovskite from ab initio Molecular Dynamics
title_sort elastic properties of casio3 perovskite from ab initio molecular dynamics
topic perovskite
first-principles calculation
seismic wave velocity
url http://www.mdpi.com/1099-4300/15/10/4300
work_keys_str_mv AT shigeakiono elasticpropertiesofcasio3perovskitefromabinitiomoleculardynamics