Journal
PHYSICAL CHEMISTRY CHEMICAL PHYSICS
Volume 24, Issue 47, Pages 29205-29213Publisher
ROYAL SOC CHEMISTRY
DOI: 10.1039/d2cp04209f
Keywords
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Funding
- Spanish National Research Agency (AEI)
- Principado de Asturias (FICYT)
- FEDER
- [PGC2018-094814-B-C22]
- [PID2021-122585NB-C21]
- [RED2018-102612-T]
- [AYUD/2021/51036]
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This study reveals the phase transition mechanism of alkaline-earth carbonates through calculation and molecular dynamics simulation, and contributes to the understanding of the role of carbonates in the Earth's interior.
To advance in the understanding of the Earth's carbon cycle, it is necessary to determine thermodynamic boundaries and kinetic barriers associated with the pressure-induced polymorphic sequence of alkaline-earth carbonates. Following a symmetry-based strategy within the martensitic approximation, we propose a two-step mechanism mediated by a hexagonal P6(3)/mmc structure for the aragonite to post-aragonite transformation in the MCO3 (M = Ca, Sr, Ba) crystal family. The calculated transition pressures and activation energies, from similar to 7 to 42 GPa and similar to 0.3 to 0.6 eV, respectively, are low enough to allow this transformation to occur under mantle conditions. Our analysis reveals that the intermediate hexagonal structure is the early one proposed by Holl et al., Phys. Chem. Miner., 2000, 27, 467-473 for high pressure BaCO3, and later considered as metastable. Phonon calculations inform that this P6(3)/mmc structure is in fact unstable at zero pressure. Remarkably, our molecular dynamics calculations showed that this instability smoothly leads to a dynamically stable P6(3)mc structure, which we confirm is actually the phase observed by Holl et al. This finding allows us to reconcile previous controversial data and contributes to clarifying the role of carbonates in the Earth's interior.
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