Towards in situ Calculation of Nucleosynthesis in Supernova Models

Details Towards in situ Calculation of Nucleosynthesis in Supernova Models Towards in situ Calculation of Nucleosynthesis in Supernova Models

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005oicc.conf..391j&link_type=abstract

OPEN ISSUES IN CORE COLLAPSE SUPERNOVA THEORY . Held 22-24 June 2004 in National Institute for Nuclear Theory, University of Was

Physics

Nuclear Physics

Nuclear Theory

2

Scientific paper

We have constructed a matrix solver for large-scale sparse matrices that arise from the treatment of nuclear burning in convective or advective environments in one dimension. We use this solver to compute nuclear abundances in a parameterized problem relevant for nucleosynthesis in supernova explosions. We discuss some details of our solutions, possible future extensions to higher dimensionality, and possible inclusion in supernova codes themselves.

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