Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
F Rizzuti,
R Hirschi,
V Varma
et al.
Abstract:One-dimensional (1D) stellar evolution models are widely used across various astrophysical fields, however they are still dominated by important uncertainties that deeply affect their predictive power. Among those, the merging of independent convective regions is a poorly understood phenomenon predicted by some 1D models but whose occurrence and impact in real stars remain very uncertain. Being an intrinsically multi-D phenomenon, it is challenging to predict the exact behaviour of shell mergers with 1D models… Show more
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