October 13, 2025Open Access

The Interplay between Dust Dynamics and Turbulence Induced by the Vertical Shear Instability

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Dust concentration enhances in vortices created by the Rossby wave instability, increasing the likelihood of planetesimal formation.
Protoplanetary disks show weakened vertical shear instability effects due to dust back-reaction, while streaming instability remains unaffected.
Models demonstrate dust settles more with increased buoyancy, suppressing turbulence caused by vertical shear instability.
Higher resolution simulations are necessary to fully understand how dust clumping develops in protoplanetary disks.

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Implication

This study demonstrates dust concentration and turbulence effects in protoplanetary disks, suggesting dust dynamics play a critical role in planet formation.

Cite This Study

Huang et al. (2025) studied this question.

synapsesocial.com/papers/68ece2abd1bb2827d1297321 https://doi.org/10.48550/arxiv.2503.01656

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Implication

This study demonstrates dust concentration and turbulence effects in protoplanetary disks, suggesting dust dynamics play a critical role in planet formation.

The Interplay between Dust Dynamics and Turbulence Induced by the Vertical Shear Instability

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Implication

Cite This Study

The Interplay between Dust Dynamics and Turbulence Induced by the Vertical Shear Instability

Key Points

Discussion

Implication

Cite This Study

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