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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 21.

Temporal summations of released energy through nuclear reactions. Results from the network calculation (thick lines) and pseudo-flashing method (thin lines) are shown for three flows. The solid thin line (flow-A calculated with the pseudo-flashing method) presents almost the same evolution as the network case and is hidden by the solid thick line.

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