Vertical shear instability in the solar nebula
arXiv:1603.01615 · doi:10.1017/S174392131500589X
Abstract
We quantify the thermodynamic requirement for the Vertical Shear Instability and evaluate its relevance to realistic protoplanetary disks as a potential route to hydrodynamic turbulence.
IAUS 314 proceedings, main paper arXiv:1505.02163