Two saturated states of the vertical shear instability in protoplanetary disks with vertically varyi...
Two saturated states of the vertical shear instability in protoplanetary disks with vertically varying cooling times
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Turbulence in protoplanetary disks plays an important role in dust evolution and planetesimal formation. The vertical shear instability (VSI) is one of the candidate hydrodynamic mechanisms that can generate turbulence in the outer disk regions. The VSI requires rapid gas cooling in addition to vertical shear. A linear stability analysis suggests t...
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Two saturated states of the vertical shear instability in protoplanetary disks with vertically varying cooling times
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TN_cdi_proquest_journals_2747749800
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2747749800
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2212.02743
