High-pressure order-disorder transition in Mg2SiO4: implications for super-Earth mineralogy

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dc.contributor.author Dutta, Rajkrishna
dc.contributor.author Tracy, Sally J.
dc.contributor.author Cohen, R. E.
dc.coverage.spatial United States of America
dc.date.accessioned 2023-02-09T14:23:47Z
dc.date.available 2023-02-09T14:23:47Z
dc.date.issued 2023-01
dc.identifier.citation Dutta, Rajkrishna; Tracy, Sally J. and Cohen, R. E., "High-pressure order-disorder transition in Mg2SiO4: implications for super-Earth mineralogy", arXiv, Cornell University Library, DOI: arXiv:2301.12701, Jan. 2023. en_US
dc.identifier.uri http://arxiv.org/abs/2301.12701
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/8559
dc.description.abstract (Mg, Fe)SiO3 post-perovskite is the highest pressure silicate mineral phase in the Earth's interior. The extreme pressure and temperature conditions inside large extrasolar planets will likely lead to phase transitions beyond pPv. In this work we have explored the high-pressure phase relations in Mg2SiO4 using computations based on density functional theory. We find that a partially disordered I-42d type structure would be stable in the interiors of these super-Earth planets. The discovery of a structure where two very dissimilar cations, Mg2+ and Si4+ occupy the same crystallographic site opens up a domain of interesting crystal chemistry and provides a foundation for other silicates and oxides with mixed occupancy. We have explored the mechanism of the phase transition from the ordered ground state and the effect of the disordering on electronic properties of the silicate phase.
dc.description.statementofresponsibility by Rajkrishna Dutta, Sally J. Tracy and R. E. Cohen
dc.language.iso en_US en_US
dc.publisher Cornell University Library en_US
dc.subject Silicate mineral phase en_US
dc.subject Density functional theory en_US
dc.subject Crystallography en_US
dc.subject Phase transitions en_US
dc.subject Super-earth en_US
dc.title High-pressure order-disorder transition in Mg2SiO4: implications for super-Earth mineralogy en_US
dc.type Pre-Print Archive en_US
dc.relation.journal arXiv


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