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Revisiting Impacts of Nuclear Burning for Reviving Weak Shocks in Neutrino-driven Supernovae

  • Authors: Ko Nakamura, Tomoya Takiwaki, Kei Kotake, and Nobuya Nishimura

Nakamura et al. 2014 The Astrophysical Journal 782 91.

  • Provider: AAS Journals

Caption: Figure 10.

Parameter maps of the initial neutrino luminosity L ν0, 52 and its decay time t d that separates the non-exploding regime (blue region) from the exploding one (red region) in 1D simulations for the four different progenitors. A horizontal yellow region inbetween (clearly visible for the LC15 progenitor; top left) shows the parameter region in which 1D explosions are obtained when the network calculation is performed.

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