Abstract
The stability of possible termination structures for the (010) surface of forsterite, Mg2SiO4, is studied using a density functional theory (DFT)-based thermodynamic approach. The DFT calculations are used to estimate the surface Gibbs free energy of various surface structures and compare their stability as a function of the chemical environment. Among nine possible terminations, the SiO-II, M2, and O-II terminations are found to be most stable as conditions range from Mg-poor to Mg-rich. This relative stability order remains the same at elevated temperatures. The surface phase diagram obtained provides ground for further theoretical studies of chemical processes on forsterite surfaces in terrestrial planets.
| Original language | English |
|---|---|
| Journal | Journal of Physical Chemistry C |
| Volume | 123 |
| Issue number | 1 |
| Pages (from-to) | 464-472 |
| ISSN | 1932-7447 |
| DOIs | |
| Publication status | Published - 2019 |
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