Fig. 2 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. 2.

Plots of density and entropy vs. radius comparing one‐dimensional simulations with our PPM and MGFLD codes, at 307 ms after the start of our run. (b) Plots of electron fraction and radial velocity vs. radius for the same comparison shown in (a). (c) Plots of density and entropy vs. radius comparing one‐dimensional simulations with our PPM and MGFLD codes, at 512 ms after the start of our run. (d) Plots of electron fraction and radial velocity vs. radius for the same comparison shown in (c).

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