Multidimensional, multiphysics simulations of core—collapse supernovae

Details Multidimensional, multiphysics simulations of core—collapse supernovae Multidimensional, multiphysics simulations of core—collapse supernovae

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jphcs.125a2010m&link_type=abstract

Journal of Physics: Conference Series, Volume 125, Issue 1, pp. 012010 (2008).

Physics

5

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 review the code's architecture and some recently improved implementations used in the code. We also briefly discuss preliminary results obtained with the code in three spatial dimensions.

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