Probing the critical point of MgSiO3 using deep potential simulation

Author:

Xu Fei-Yang12ORCID,Li Zhi-Guo2ORCID,Chen Xiang-Rong1ORCID,Geng Hua Y.2ORCID,Liu Lei3ORCID,Hu Jianbo2ORCID

Affiliation:

1. College of Physics, Sichuan University 1 , Chengdu 610065, China

2. National Key Laboratory for Shock Wave and Detonation Physics Research, Institute of Fluid Physics, CAEP 2 , Mianyang 621900, China

3. School of Science, Southwest University of Science and Technology 3 , Mianyang 621010, China

Abstract

The giant impact between proto-Earth and a Mars-sized planet called Theia resulted in the formation of the Earth–Moon system, and the silicate mantles of the initial bodies may have partly been vaporized. Here, we develop a machine learning potential for MgSiO3 based on the data from first-principles calculations to estimate its critical point. The variations in pressure along different isotherms yield the position of the critical point of MgSiO3 at 0.54 g cm−3 and 6750 ± 250 K, which agrees with the previous theoretical estimation. We also simulate the MgSiO3 melt under a spectrum of critical conditions to understand the changes in coordination environment with density and temperature. The fourfold Si–O coordination hardly changes with increasing density at 3000 K. However, with increasing temperature, the dominance of four-coordinated Si–O diminishes rapidly as density decreases. Regarding Mg–O coordination, the overall trend, which varies with temperature and density, remains largely consistent with Si–O but with a greater diversity in the types of coordination due to more bond breaking events. Our work opens a new avenue by employing machine learning methods to estimate the critical point of silicates.

Funder

National Natural Science Foundation of China

Sichuan Province Science and Technology Support Program

Publisher

AIP Publishing

Reference43 articles.

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