Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network

Open Access

Fig. 14.

Position for the pre-supernova models in the (M₄ ⋅ μ₄, μ₄) plane. The blue and magenta lines are separating likely explosions (below the line) and likely black hole formation (above the line). The parametric lines are taken from Ertl et al. (2016). The blue line corresponds to the calibration using the s19.8 model (Eq. (27)) and the magenta line to the w20 model (Eq. (28)).

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