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This is a Hydrodynamical simulations study.

September 10, 2025Astronomy and Astrophysics

Hydrodynamical simulations of the vertical shear instability with dynamic dust and cooling rates in protoplanetary disks

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Dust distribution varies under the influence of turbulence from the vertical shear instability.
Simulations indicate an equilibrium state forms with dust settling and turbulence balance reached.
The effectiveness of dust growth and mixing is influenced by dust size and dust-to-gas mass ratio.
Cooling rates and the dynamics of dust play critical roles in forming thick dust layers in protoplanetary disks.

Authors

YFYuya FukuharaTokyo Institute of Technology MFMario FlockMax Planck Institute for Astronomy SOSatoshi OkuzumiTokyo Institute of Technology

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Implication

Observational analysis of vertical shear instability's influence on dust dynamics in protoplanetary disks, indicating dust distribution is affected by turbulence and cooling rates.

Cite This Study

Fukuhara et al. (2025) studied this question.

synapsesocial.com/papers/68c19f9c54b1d3bfb60db3f0 https://doi.org/10.1051/0004-6361/202555624

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Implication

Observational analysis of vertical shear instability's influence on dust dynamics in protoplanetary disks, indicating dust distribution is affected by turbulence and cooling rates.

Hydrodynamical simulations of the vertical shear instability with dynamic dust and cooling rates in protoplanetary disks

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Discussion

Implication

Cite This Study

Hydrodynamical simulations of the vertical shear instability with dynamic dust and cooling rates in protoplanetary disks

Key Points

Discussion

Implication

Cite This Study

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