Superionic silica-water and silica-hydrogen compounds under high pressure

TL;DR

This study discovers superionic silica-water and silica-hydrogen compounds under extreme pressures, revealing their potential role in planetary interiors and magnetic fields of giant planets like Uranus and Neptune.

Contribution

It identifies new superionic compounds in the Si-O-H system at high pressures and explores their implications for planetary science.

Findings

Silica-water compound (SiO2)2(H2O) exists above 450 GPa.

Silica-hydrogen compound SiO2H2 exists above 650 GPa.

These compounds exhibit superionic behavior at planetary interior conditions.

Abstract

Silica, water and hydrogen are known to be the major components of celestial bodies, and have significant influence on the formation and evolution of giant planets, such as Uranus and Neptune. Thus, it is of fundamental importance to investigate their states and possible reactions under the planetary conditions. Here, using advanced crystal structure searches and first-principles calculations in the Si-O-H system, we find that a silica-water compound (SiO2)2(H2O) and a silica-hydrogen compound SiO2H2 can exist under high pressures above 450 and 650 GPa, respectively. Further simulations reveal that, at high pressure and high temperature conditions corresponding to the interiors of Uranus and Neptune, these compounds exhibit superionic behavior, in which protons diffuse freely like liquid while the silicon and oxygen framework is fixed as solid. Therefore, these superionic silica-water and silica-hydrogen compounds could be regarded as important components of the deep mantle or core of giants, which also provides an alternative origin for their anomalous magnetic fields. These unexpected physical and chemical properties of the most common natural materials at high pressure offer key clues to understand some abstruse issues including demixing and erosion of the core in giant planets, and shed light on building reliable models for solar giants and exoplanets.