Multi-Angle Multi-Group Radiation-Hydrodynamics Simulations Of Core-Collapse Supernovae

Details Multi-Angle Multi-Group Radiation-Hydrodynamics Simulations Of Core-Collapse Supernovae Multi-Angle Multi-Group Radiation-Hydrodynamics Simulations Of Core-Collapse Supernovae

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aps..apr.s1011o&link_type=abstract

American Physical Society, 2008 APS April Meeting and HEDP/HEDLA Meeting, April 11-15, 2008, abstract #S1.011

Physics

Scientific paper

We present new results from axisymmetric multi-angle, multi-group neutrino radiation-hydrodynamic calculations of the postbounce phase of rotating and nonrotating core-collapse supernovae. We analyze the effect of the multi-angle treatment on neutrino radiation field anisotropies and the net energy deposition and compare our results in detail with multi-group flux-limited diffusion counterpart calculations.

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