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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 19.

Schematic picture of ρ– T plane characterizing our pseudo-flashing method. Region I almost consists of nickel, region II contains α-particles and free nucleons, and in region III all nuclei and α-particles are dissolved into free nucleons. In region IV we resolve the nuclear network to evolve the chemical compositions. See Rampp & Janka (2002) for details. We take three flows (A, B, and C) as representations of mass shells in the LC15 model.

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