Figure 2 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 2.

Time evolution of the shock radii for model LC15 with different initial neutrino luminosities ( L _{ν0, 52} in unit of 10 ⁵² erg s ⁻¹) and the decay time ( t _d in unit of s). The red and blue lines correspond to the results with and without the energy feedback from nuclear reactions, respectively.

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