12The temperature variations on top of the core-mantle boundary are governed by the 13 thermal conductivity of the minerals that comprise the overlying mantle. Estimates of the 14 thermal conductivity of the most abundant phase, MgSiO 3 perovskite, at core-mantle 15 boundary conditions vary by a factor of ten. We performed ab initio simulations to 16 determine the lattice thermal conductivity of MgSiO 3 perovskite, finding a value of 6.8 ± 0.9 17 W m -1 K -1 at core-mantle boundary conditions (136 GPa and 4000 K), consistent with 18 geophysical constraints for the thermal state at the base of the mantle. Thermal 19 conductivity depends strongly on pressure, explaining the dynamical stability of super-20 plumes. The dependence on temperature and composition is weak in the deep mantle: our 21 results exhibit saturation as the phonon mean free path approaches the interatomic 22 spacing. Combining our results with seismic tomography, we find large lateral variations in 23 the heat-flux from the core that have important implications for core dynamics. 24
Keywords 25MgSiO 3 perovskite; thermal conductivity; mantle dynamics 26 27