Figure 16 from Revisiting Impacts of Nuclear Burning for Reviving Weak Shocks in Neutrino-driven Supernovae

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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 16.

Time evolution of the diagnostic energy (red line) and net nuclear burning energy (green) for LC15 model in 2D ( n _θ = 32) with ( L _{ν0, 52}, t _d ) = (2.4, 3.0). The diagnostic energy of the case without nuclear burning (blue) is also shown.

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