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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 6.

Time evolution of diagnostic energy is shown for the same model as Figure 5. The green line is the energy released by nuclear burning and the diagnostic energy without nuclear burning (blue) is also shown. Here the diagnostic energy is defined as the sum of the kinetic, thermal, and gravitational energy of fluid elements with positive radial velocity.

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