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Dynamics / Taylor–Couette flow / Magnetorotational instability / Turbulence / Hydrodynamic stability / Accretion disc / Reynolds number / Reynolds stress / Couette flow / Fluid dynamics / Physics / Fluid mechanics
Date: 2006-11-15 15:09:40
Dynamics
Taylor–Couette flow
Magnetorotational instability
Turbulence
Hydrodynamic stability
Accretion disc
Reynolds number
Reynolds stress
Couette flow
Fluid dynamics
Physics
Fluid mechanics

Vol 444 | 16 November 2006 | doi:nature05323 LETTERS Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks Hantao Ji1, Michael Burin1{, Ethan Schartman1 & Jeremy Goodman1

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