Intermediate spin state and the B1-B2 transition in ferropericlase at tera-Pascal pressures
Ferropericlase (fp), (Mg\(_{1-x}\)Fe\(_x\))O, the second most abundant mineral in the Earth's lower mantle, is expected to be an essential component of super-Earths' mantles. Here we present an ab initio investigation of the structure and magnetic ground state of fp up to \(\sim\) 3 TPa wi...
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Veröffentlicht in: | arXiv.org 2022-05 |
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Sprache: | eng |
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Zusammenfassung: | Ferropericlase (fp), (Mg\(_{1-x}\)Fe\(_x\))O, the second most abundant mineral in the Earth's lower mantle, is expected to be an essential component of super-Earths' mantles. Here we present an ab initio investigation of the structure and magnetic ground state of fp up to \(\sim\) 3 TPa with iron concentrations (x\(_{Fe}\)) varying from 0.03 to 0.12. Calculations were performed using LDA+U\(_{sc}\) and PBE exchange-correlation functionals to elucidate the pressure range for which the Hubbard U (U\(_{sc}\)) is required. Similar to the end-members FeO and MgO, fp also undergoes a B1 to B2 phase transition that should be essential for modeling the structure and dynamics of super-Earths' mantles. This structural transition involves a simultaneous change in magnetic state from a low spin (LS) B1 phase with iron total spin S=0 to an intermediate spin (IS) B2 phase with S=1. This is a rare form of pressure/strain-induced magnetism produced by local cation coordination changes. Phonon calculations confirm the dynamical stability of the iron B2-IS state. Free energy calculations are then carried out including vibrational effects and electronic and magnetic entropy contributions. The phase diagram is then obtained for low concentration fp using a quasi-ideal solid solution model. For x\(_{Fe}\) > 0.12 this approach is no longer valid. At ultra-high pressures, there is an IS to LS spin state change in Fe in the B2 phase, but the transition pressure depends sensitively on thermal electronic excitations and on x\(_{Fe}\). |
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ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.2109.11008 |