Fig. 1.

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Peak shock temperature (solid red lines) and velocity (solid green lines) for different initial explosive conditions in the 20 M⊙ progenitor from Ritter et al. (2018b). The purple line represents the logarithm of the quantity ρr3 in the pre-supernova model in arbitrary units. The gray region represents the temperature range for the activation of the γ process, i.e., between 2 GK and 3.5 GK. Note that the saturation of the shock velocity at ∼4.2 M⊙ at the value of 5 × 109 cm s−1 is due to the artificial cap imposed for viscous forces (see Sect. 2.1).
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