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High-resolution Three-dimensional Simulations of Core-collapse Supernovae in Multiple Progenitors

  • Authors: Sean M. Couch and Evan P. O'Connor

Couch & O'Connor 2014 The Astrophysical Journal 785 123.

  • Provider: AAS Journals

Caption: Figure 5.

Net neutrino heating in the gain region (top), heating efficiency, (middle), and mass in the gain region (bottom) for s15 (left) and s27(right). At early times ( t pb < 50 ms), before significant non-spherical motion as developed in 2D and 3D, these metrics are very similar for all models with the same heat factor.

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