Missing Mixing?

Astronomy and Astrophysics – Astronomy

Scientific paper

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Convection, Hydrodynamics, Stars: Evolution, Stars: Interiors, Stars: Rotation

Scientific paper

Shear-generated turbulent mixing in stellar radiative regions (stably stratified) has recently been found to be too weak. This has stimulated the search for the missing mixing. We suggest that there may not be a missing mixing problem. Phenomenological models have underestimated its real strength, thus leading to a negative assessment of its real potential.

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