Novel stable compounds in the Mg-O system under high pressure
Qiang Zhu1, Artem R Oganov, Andriy O Lyakhov
1Department of Geosciences, Stony Brook University, Stony Brook, New York 11794, USA. qiang.zhu@stonybrook.edu
Physical Chemistry Chemical Physics : PCCP
|April 19, 2013
Summary
High-pressure magnesium oxide (MgO) research reveals two new stable compounds, MgO2 and Mg3O2. These discoveries offer insights into materials science and planetary interiors under extreme conditions.
Area of Science:
- Materials Science
- High-Pressure Physics
- Computational Chemistry
Background:
- The magnesium-oxygen (Mg-O) system is fundamental to understanding planetary interiors and material properties under extreme conditions.
- Previous studies have primarily focused on magnesium oxide (MgO), with limited exploration of other stoichiometries at high pressures.
Purpose of the Study:
- To computationally explore the full range of possible stoichiometries for the Mg-O system at pressures up to 850 GPa.
- To identify novel thermodynamically stable Mg-O compounds and analyze their chemical bonding and electronic properties.
Main Methods:
- Utilized ab initio evolutionary simulations to predict stable Mg-O phases.
- Performed detailed chemical bonding analysis, including charge transfer and electron density distribution.
- Calculated electronic band structures to determine material conductivity.
Main Results:
- Identified two new thermodynamically stable compounds: MgO2 at 116 GPa and Mg3O2 at 500 GPa, in addition to MgO.
- MgO2 exhibits peroxide ions [O-O](2-), while Mg3O2 is an electride with non-nuclear electron density maxima acting as anions.
- Mg3O2 possesses a significantly narrower band gap compared to MgO and MgO2, suggesting potential semiconducting properties.
Conclusions:
- The Mg-O system hosts novel stable compounds (MgO2, Mg3O2) under high pressure, expanding known magnesium oxide phases.
- The unique bonding in MgO2 and Mg3O2, including peroxide and electride characteristics, highlights complex chemistry at extreme conditions.
- These findings provide a basis for understanding the existence and properties of Mg-O compounds within planetary interiors.
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