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The impact of large-scale turbulence on the redistribution of angular momentum in stellar accretion disks
Authors:Ye P Velikhov  A Yu Lugovsky  S I Mukhin  Yu P Popov  V M Chechetkin
Institution:(1) Kurchatov Institute Russian Research Centre, Kurchatov sq. 1, Moscow, 123182, Russia;(2) Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Miusskaya pl. 4, Moscow, 125047, Russia;(3) Moscow State University, Vorob’evy gory, Moscow, 119899, Russia
Abstract:We consider the origin and development of large-scale turbulence in a shear flow in a stellar accretion disk. The ratio of the kinetic energy of vortices originating in the turbulent flow and the total initial kinetic energy of the rotating disk is essentially constant. The large-scale structures that form are able to redistribute the angular momentum without any appreciable heating of the matter.
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