113 / 2023-04-13 22:32:58
Thermal Conductivity of MgSiO3 under Lower Mantle Conditions Calculated by Machine Learning Potential
Thermal conductivity,Lower mantle,MgSiO3,Machine learning potential
Abstract Accepted
Xiaoxiang Yu / Natianal University of Defense Technology
Fenghu Yang / National University of Defense Technology
Qiyu Zeng / National University of Defense Technology
Jiayu Dai / National University of Defense Technology
Thermal conduction of mantle minerals determines the magnitude of heat flux across the core-mantle boundary and is related to the thermal dynamics and evolution of the core and mantle, the formation and stability of the mantle plumes, and the generation of the magnetic field [1-3]. Therefore, the thermal conductivity κ of MgSiO3 (the most abundant mineral in the Earth’s lower mantle) is an important parameter in determining the heat budget of the Earth. Experimental measurement of κ under extreme conditions is still controversial and challenging [4,5]. Theoretical calculation based on the phonon gas model (PGM), in which a phonon is considered a quasiparticle, may underestimate the κ due to the failure of the phonon quasiparticle picture. In low-κ materials, a number of phonons are referred to as ill-defined phonons, for example, whose mean free paths are shorter than the Ioffe–Regel limit [6]. In this work [7], to deal with the ill-defined phonons, molecular dynamics (MD) simulations are used to obtain the κ under lower mantle conditions. We train a machine learning deep potential (DP) model [8] based on density functional theory datasets to accurately capture the interatomic interactions over a wide P-T range. Compared with previous PGM results [9], the κ predicted by DPMD is larger at low P and high T and closer to the experimental value [4]. The discrepancy is attributed that the contribution of ill-defined phonons is underestimated in the PGM but included in DPMD simulations. A larger κ of MgSiO3 predicted by DPMD would imply a thicker boundary layer and more stable mantle plumes. Our results emphasize the significance of ill-defined phonons and would provide thermophysical data for evaluating the thermal dynamics and improving the Earth model.
Important Date
  • Conference Date

    Jun 05

    2023

    to

    Jun 09

    2023

  • Apr 30 2023

    Early Bird Registration

  • May 01 2023

    Abstract Submission Deadline

  • May 01 2023

    Abstract Notification of Acceptance

  • May 01 2023

    Draft paper submission deadline

  • May 31 2023

    Registration deadline

Sponsored By
Science and Technology on Plasma Physics Laboratory
Department of Astronomy, Beijing Normal University
Organized By
Matter and Radiation at Extremes
Institute of Fluid Physics, China Academy of Engineering Physics, China
Institute of Applied Physics and Computational Mathematics, Beijing, China
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