Angular momentum extraction by gravity waves in the Sun
Suzanne Talon, Pawan Kumar, Jean-Paul Zahn
Abstract
We review the behavior of the oscillating shear layer produced by gravity waves below the surface convection zone of the Sun. We show that, under asymmetric filtering produced by this layer, gravity waves of low spherical order, which are stochastically excited at the base of the convection zone of late type stars, can extract angular momentum from their radiative interior. The time-scale for this momentum extraction in a Sun-like star is of the order of 107 years. The process is particularly efficient in the central region, and it could produce there a slowly rotating core.
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