Image Details

Choose export citation format:

Large resolution
Export to PDF PPT Format

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. 10.

(a) Plots of the angle‐averaged d∊/dt at 137, 212, and 512 ms after bounce; d∊/dt is the net heating or cooling from electron neutrino and antineutrino absorption and emission. (b) Plots of the maximum net neutrino heating and maximum net neutrino cooling rates as a function of time during the course of our simulation. (c) Plots of the maximum net neutrino heating and maximum net neutrino cooling rates as a function of time during the critical 50–150 ms after bounce.

Other Images in This Article

Show More

Copyright and Terms & Conditions