2023
DOI: 10.1038/s41586-023-06215-0
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Variation in bridgmanite grain size accounts for the mid-mantle viscosity jump

Abstract: A viscosity jump of one to two orders of magnitude in the lower mantle of Earth at 800–1,200-km depth is inferred from geoid inversions and slab-subducting speeds. This jump is known as the mid-mantle viscosity jump1,2. The mid-mantle viscosity jump is a key component of lower-mantle dynamics and evolution because it decelerates slab subduction3, accelerates plume ascent4 and inhibits chemical mixing5. However, because phase transitions of the main lower-mantle minerals do not occur at this depth, the origin o… Show more

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Cited by 3 publications
(5 citation statements)
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“…Our calculation shows that grain growth under the static conditions is too slow to reach sizes (i.e., ∼3 cm) that give high viscosity particularly at the shallow depths (i.e., 1,000–2,000 km) in Mitrovica and Forte (2004). In a recent study (Fei et al., 2023), portions of the lower mantle with high viscosity were considered to have a small fraction of ferropericlase (i.e., f II < 0.05–0.1) that promotes grain growth via reduced grain boundary pinning, which in turn increases mantle viscosity. Based on the relationship dfII0.5 $d\propto {{f}_{\text{II}}}^{-0.5}$ (Equation 3), at T +200/+200 K for 4.5 billion years and at the shallow depths of 1,000–2,000 km, the final grain size is 6–20 mm, even for a very small ferropericlase fraction of 2 vol%.…”
Section: Discussionmentioning
confidence: 99%
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“…Our calculation shows that grain growth under the static conditions is too slow to reach sizes (i.e., ∼3 cm) that give high viscosity particularly at the shallow depths (i.e., 1,000–2,000 km) in Mitrovica and Forte (2004). In a recent study (Fei et al., 2023), portions of the lower mantle with high viscosity were considered to have a small fraction of ferropericlase (i.e., f II < 0.05–0.1) that promotes grain growth via reduced grain boundary pinning, which in turn increases mantle viscosity. Based on the relationship dfII0.5 $d\propto {{f}_{\text{II}}}^{-0.5}$ (Equation 3), at T +200/+200 K for 4.5 billion years and at the shallow depths of 1,000–2,000 km, the final grain size is 6–20 mm, even for a very small ferropericlase fraction of 2 vol%.…”
Section: Discussionmentioning
confidence: 99%
“…This result does not support our prediction of δDGB_gr ${\delta D}_{\text{GB}\_\text{gr}}$, which should be approximately equal to the diffusivity of the slowest species, that is, 5δDSi_BrGB $5\delta {D}_{\text{Si}\_\text{BrGB}}$ (Equation 6). At present, there is no good explanation for the fact that the diffusivities predicted from the grain growth rates (Fei et al., 2021, 2023) are larger than the measured self‐diffusivities (Dobson et al., 2008; Yamazaki et al., 2000). Parameters for estimating δD comGB and D comLatt over a wide range of pressures and temperatures in the lower mantle are known in more detail from the diffusion studies.…”
Section: Grain Growth and Creep Of The Lower Mantle Materialsmentioning
confidence: 90%
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