First-principles study of the lattice thermal conductivity of MgSiO<sub>3</sub> akimotoite in the mantle transition zone
The lattice thermal conductivity (<inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula>) of mantle minerals plays a crucial role in the heat flow and temperature distribution within the Earth. MgSiO<sub>3</sub> akimotoite is stable at the bottom of the mantle transition zone; it transitions to MgSiO<sub>3</sub> perovskite (MgPv). In this work, we carry out a study of the <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula> of MgSiO<sub>3</sub> akimotoite for pressures up to 25 GPa and temperatures up to 2500 K, based on first-principles calculations combined with lattice dynamics theory. At 300 K and 25 GPa, the <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula> of MgSiO<sub>3</sub> akimotoite is 37.66 W m<sup>–1</sup> K<sup>–1</sup>, larger than that of MgPv (13.46 W m<sup>–1</sup> K<sup>–1</sup>), which implies that the phase transition explains the reduction in <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula>. At 300 K, the pressure dependence of <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula> is 0.68 W m<sup>–1</sup> K<sup>–1</sup> GPa<sup>-1</sup>, stronger than that of MgPv (0.48 W m<sup>–1</sup> K<sup>–1</sup> GPa<sup>-1</sup>). The azimuthal anisotropy in <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula>of MgSiO<sub>3</sub> akimotoite decreases from 45.5% at 0 GPa to 28.94% at 25 GPa, while the variation trend is opposite to that of MgPv. In MgSiO<sub>3</sub> akimotoite, Fe incorporating in the mineral leads to a decrease in <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula> and an increase in azimuthal anisotropy. Along the geotherm, the <inline-formula><span class="inline-formula-span">\kappa _\rmlatt</span><img text_id='M1' class='formula-img' style='display:none;' src='RA566-zhangli-F_M1.jpg'><alternatives></alternatives></inline-formula> of MgSiO<sub>3</sub> akimotoite is lower than that of ringwoodite, which would suggest that MgSiO<sub>3</sub> akimotoite slows down heat conduction at the bottom of mantle transition zone. These findings are useful for determining the thermal structure of, and understanding heat transfer in, the interior of the Earth.
Authors
- Qiuyun Chen (ORCID: https://orcid.org/0000-0003-1866-1125)
- Hong Zheng (ORCID: https://orcid.org/0000-0001-7386-7084)
- Li Zhang (ORCID: https://orcid.org/0000-0002-4015-7665)
- Ai Lu (ORCID: https://orcid.org/0000-0001-7624-5379)
Publication Details
- Journal
- Earth and Planetary Physics
- Published
- 2025-01-01
- DOI
- https://doi.org/10.26464/epp2025051
- Primary Topic
- High-pressure geophysics and materials
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Natural Science Foundation of China
- China University of Geosciences