Japan Geoscience Union Meeting 2021

Presentation information

[E] Oral

S (Solid Earth Sciences ) » S-IT Science of the Earth's Interior & Techtonophysics

[S-IT16] Structure and Dynamics of Earth and Planetary Mantles

Fri. Jun 4, 2021 3:30 PM - 4:45 PM Ch.24 (Zoom Room 24)

convener:Takashi Nakagawa(University of Leeds), Takashi Yoshino(Institute for Planetary Materials, Okayama University), Dapeng Zhao(Department of Geophysics, Tohoku University), Chairperson:Takashi Yoshino(Institute for Planetary Materials, Okayama University)

4:30 PM - 4:45 PM

[SIT16-10] First-principles prediction of order-disorder transition in Mg2GeO4

*Koichiro Umemoto1,2, Renata Wentzcovitch3 (1.Earth-Life Science Institute, Tokyo Institute of Technology, 2.RIKEN, 3.Columbia University)

Keywords:Phase transition under high pressure and temperature, super-Earth, First-principles calculation

Here we present an first-principles prediction of a temperature-induced order-disorder transition (ODT) from I-42d-type to Th3P4-type phase in I-42d-type Mg2GeO4. This uncommon type of prediction is achieved by carrying out a high-throughput sampling of atomic configurations in a 56-atom supercell followed by a Boltzmann ensemble statistics calculation. Mg2GeO4 is a low-pressure analog [1] of ultrahigh pressure I-42d-type Mg2SiO4 [2]. The latter was predicted to occur as a product of dissociation/recombination transitions in MgSiO3 post-perovskite at multi-Mbar pressures (post-PPV transitions) [3]. In the Mg-Ge-O system, this post-PPV phase occurs beyond ~150 GPa [1]. The new ODT predicted here alters the sequence of post-PPV phases in Mg2GeO4 at high temperatures (>~2,000 K) and likely also in Mg2SiO4. I-42d-type Mg2SiO4 is predicted to occur in the deep interiors of super-Earths [2-5]. Therefore, this newly found ODT should be relevant for modeling the internal dynamics and structure of super-Earth-type planets. The prediction of this Th3P4-type phase in Mg2GeO4 enhances further the relationship between the crystal structures of Earth/planet-forming silicates and oxides at extreme pressures and those of rare-earth sesquisulfides at low pressures.

References:
[1] K. Umemoto and R. M. Wentzcovitch, Phys. Rev. Materials 3, 123601 (2019).
[2] S. Q. Wu et al., J. Phys.: Condens. Matter, 26, 035402 (2014).
[3] K. Umemoto et al., Earth Planet. Sci. Lett. 478, 40-45 (2017).
[4] H. Niu et al., Scientific Reports 5, 18347 (2015).
[5] A. van den Berg, et al. Icarus 317, 412-426 (2019).