Fig. 4 from An Investigation of Neutrino‐driven Convection and the Core Collapse Supernova Mechanism Using Multigroup Neutrino Transport

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An Investigation of Neutrino‐driven Convection and the Core Collapse Supernova Mechanism Using Multigroup Neutrino Transport

Authors: A Mezzacappa, A. C. Calder, S. W. Bruenn, J. M. Blondin, M. W. Guidry, M. R. Strayer, and A. S. Umar

Mezzacappa et al. 1998 The Astrophysical Journal 495 911.

Provider: AAS Journals

Caption: Fig. 4.

(a) Two‐dimensional electron fraction plots showing the evolution of ND convection in our 15 M_☉ model, at 137, 212, and 512 ms after bounce. (b) Plots of the angle‐averaged electron fraction for the three electron fraction snapshots shown in (a). Also shown for comparison is the corresponding electron fraction from our one‐dimensional PPM simulation.

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