Simulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino Transport

Details Simulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino Transport Simulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino Transport

1997-04-17

arxiv.org/abs/astro-ph/9704181v1

Astronomy and Astrophysics

Astrophysics

Latex, using sprocl.sty, 3 pages, To appear in the proceedings of the 18th Texas Symposium on Relativistic Astrophysics

Scientific paper

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.

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