Accretion disk instability revisited. Transient dynamics of rotating shear flow

Details Accretion disk instability revisited. Transient dynamics of rotating shear flow Accretion disk instability revisited. Transient dynamics of rotating shear flow

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...425..385y&link_type=abstract

Astronomy and Astrophysics, v.425, p.385-393 (2004)

Astronomy and Astrophysics

Astrophysics

30

Accretion, Accretion Disks, Instabilities, Turbulence, Hydrodynamics

Scientific paper

Accretion disk flow in a local Cartesian (or ``shearing box'') approximation is examined for viscous three-dimensional linear disturbances. Eigenvalue computations predict that the flow is asymptotically stable unless the rotation number falls in the range 0

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