Nonlinear interaction between dynamo-generated magnetic fields, mean flows and internal gravity waves in stellar stably-stratified layers: From 3D to 1D
This paper presents a 1D mean-field model that integrates 3D-derived dynamo coefficients to demonstrate how nonlinear interactions between dynamo-generated magnetic fields and internal gravity waves create new dynamical regimes, such as magnetic perturbations of shear layer oscillations, which significantly influence angular momentum transport and the long-term rotational evolution of stellar radiative interiors.