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arXiv · 1605.09152

Drag-driven instability of a dust layer in a magnetized protoplanetary disc

Mohsen Shadmehri·Razieh Oudi·Gohar Rastegarzade
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Abstract

We study drag-driven instability in a protoplanetary disc consisting of a layer of single-sized dust particles which are coupled to the magnetized gas aerodynamically and the particle-to-gas feedback is included. We find a dispersion relation for axisymmetric linear disturbances and growth rate of the unstable modes are calculated numerically. While the secular gravitational instability in the absence of particle-to-gas feedback predicts the dust layer is unstable, magnetic fields significantly amplifies the instability if the Toomre parameter for the gas component is fixed. We also show that even a weak magnetic field is able to amplify the instability more or less irrespective of the dust-gas coupling.

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Mohsen Shadmehri, Razieh Oudi, Gohar Rastegarzade. 2016-05-30. Drag-driven instability of a dust layer in a magnetized protoplanetary disc. https://doi.org/10.1088/1674-4527/16/9/134

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