Petascale supernova simulation with CHIMERA

Details Petascale supernova simulation with CHIMERA Petascale supernova simulation with CHIMERA

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..78a2049m&link_type=abstract

Journal of Physics: Conference Series, Volume 78, Issue 1, pp. 012049 (2007).

Physics

1

Scientific paper

CHIMERA is a multi-dimensional radiation hydrodynamics code designed to study core-collapse supernovae. The code is made up of three essentially independent parts: a hydrodynamics module, a nuclear burning module, and a neutrino transport solver combined within an operator-split approach. We describe some major algorithmic facets of the code and briefly discuss some recent results. The multi-physics nature of the problem, and the specific implementation of that physics in CHIMERA, provide a rather straightforward path to effective use of multi-core platforms in the near future.

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