Simulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino Transport
arXiv:astro-ph/9704181
Abstract
In one dimension, we present results from comparisons of stationary state multigroup flux-limited diffusion and Boltzmann neutrino transport, focusing on quantities central to the postbounce shock reheating. In two dimensions, we present results from simulations that couple one-dimensional multigroup flux-limited diffusion to two-dimensional PPM hydrodynamics.
Latex, using sprocl.sty, 3 pages, To appear in the proceedings of the 18th Texas Symposium on Relativistic Astrophysics