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Nucleosynthesis in Multi-Dimensional Simulations of SNII

  • C. Travaglio
  • K. Kifonidis
  • E. Müller
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

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 15 M stars with solar metallicity, by post-processing the temperature and density history of advected tracer particles. We compare our results to 1D calculations published in the literature.

Keywords

Explosion Energy Core Collapse Supernova Marker Particle Solar Metallicity Neutrino Luminosity 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • C. Travaglio
    • 1
    • 2
  • K. Kifonidis
    • 1
  • E. Müller
    • 1
  1. 1.Max-Planck Institut für AstrophysikGarching bei MünchenGermany
  2. 2.INAF-Osservatorio Astronomico di Pino TorineseTorinoItaly

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