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

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21110517o&link_type=abstract

American Astronomical Society, AAS Meeting #211, #105.17; Bulletin of the American Astronomical Society, Vol. 39, p.931

Astronomy and Astrophysics

Astrophysics

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.
This research is funded by the Joint Institute for Nuclear Astrophysics, by the DOE/SciDAC program, and by NSF.

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