Nucleosynthesis in multi-dimensional simulations of SNII

Details Nucleosynthesis in multi-dimensional simulations of SNII Nucleosynthesis in multi-dimensional simulations of SNII

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newar..48...25t&link_type=abstract

New Astronomy Reviews, Volume 48, Issue 1-4, p. 25-30.

Astronomy and Astrophysics

Astronomy

5

Stars: Late Stages Of Evolution, Nucleosynthesis, Supernovae: Nucleosynthesis

Scientific paper

We investigate explosive nuclear burning in core collapse supernovae by coupling a tracer particle method to one- and two-dimensional Eulerian hydrodynamic calculations. Adopting the most recent experimental and theoretical nuclear data, we compute the nucleosynthetic yields for 15Msolar stars with solar metallicity, by post-processing the temperature and density history of advected tracer particles. We compare our results to one-dimensional calculations published in the literature.

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