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Capturing the Fire: Flame Energetics and Neutronization for Type Ia Supernova Simulations

  • Authors: A. C. Calder, D. M. Townsley, I. R. Seitenzahl, F. Peng, O. E. B. Messer, N. Vladimirova, E. F. Brown, J. W. Truran, and D. Q. Lamb

Calder et al. 2007 The Astrophysical Journal 656 313.

  • Provider: AAS Journals

Caption: Fig. 8.

Energy released and NSE temperature for burning C/O as functions of density of the fuel for isochoric self‐heating calculations with (solid lines) and without (dashed lines) electron screening and Coulomb corrections. For comparison, the contour corresponding to the condition (for ﹩Y_{e}=0.5﹩) that the nuclear statistical equilibrium consists of equal parts by mass of 4He and 56Ni is shown (dotted line).

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