Unveiling the effect of Ni on the formation and structure of Earth's inner core

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Sun, Yang, Mendelev, Mikhail I., Zhang, Feng, Liu, Xun, Da, Bo, Wang, Cai-Zhuang, Wentzcovitch, Renata M., Ho, Kai-Ming
Format: Preprint
Veröffentlicht: 2023
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866911760662921216
author Sun, Yang
Mendelev, Mikhail I.
Zhang, Feng
Liu, Xun
Da, Bo
Wang, Cai-Zhuang
Wentzcovitch, Renata M.
Ho, Kai-Ming
author_facet Sun, Yang
Mendelev, Mikhail I.
Zhang, Feng
Liu, Xun
Da, Bo
Wang, Cai-Zhuang
Wentzcovitch, Renata M.
Ho, Kai-Ming
contents Ni is the second most abundant element in the Earth's core. Yet, its effects on the inner core's structure and formation process are usually disregarded because of its electronic and size similarity with Fe. Using ab initio molecular dynamics simulations, we find that the bcc phase can spontaneously crystallize in liquid Ni at temperatures above Fe's melting point at inner core pressures. The melting temperature of Ni is shown to be 700-800 K higher than that of Fe at 323-360 GPa. hcp, bcc, and liquid phase relation differ for Fe and Ni. Ni can be a bcc stabilizer for Fe at high temperatures and inner core pressures. A small amount of Ni can accelerate Fe's crystallization at core pressures. These results suggest Ni may substantially impact the structure and formation process of the solid inner core.
format Preprint
id arxiv_https___arxiv_org_abs_2308_04280
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Unveiling the effect of Ni on the formation and structure of Earth's inner core
Sun, Yang
Mendelev, Mikhail I.
Zhang, Feng
Liu, Xun
Da, Bo
Wang, Cai-Zhuang
Wentzcovitch, Renata M.
Ho, Kai-Ming
Materials Science
Geophysics
Ni is the second most abundant element in the Earth's core. Yet, its effects on the inner core's structure and formation process are usually disregarded because of its electronic and size similarity with Fe. Using ab initio molecular dynamics simulations, we find that the bcc phase can spontaneously crystallize in liquid Ni at temperatures above Fe's melting point at inner core pressures. The melting temperature of Ni is shown to be 700-800 K higher than that of Fe at 323-360 GPa. hcp, bcc, and liquid phase relation differ for Fe and Ni. Ni can be a bcc stabilizer for Fe at high temperatures and inner core pressures. A small amount of Ni can accelerate Fe's crystallization at core pressures. These results suggest Ni may substantially impact the structure and formation process of the solid inner core.
title Unveiling the effect of Ni on the formation and structure of Earth's inner core
topic Materials Science
Geophysics
url https://arxiv.org/abs/2308.04280