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Nucleosynthesis in Multi-Dimensional Simulations of SNII

Published online by Cambridge University Press:  19 September 2016

C. Travaglio ,
K. Kifonidis  and
E. Müller
C. Travaglio
Affiliation:
Max-Planck Institut für Astrophysik, Karl-Scwarzschild Str. 1, 85741 Garching bei München, Germany INAF-Osservatorio Astronomico di Pino Torinese, Strada Osservatorio 20, 10025 Torino, Italy;travaglio@to.astro.it
K. Kifonidis
Affiliation:
Max-Planck Institut für Astrophysik, Karl-Scwarzschild Str. 1, 85741 Garching bei München, Germany
E. Müller
Affiliation:
Max-Planck Institut für Astrophysik, Karl-Scwarzschild Str. 1, 85741 Garching bei München, Germany

Summary

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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.

Type
Part IV Supernovae: Models
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 297 - 301
Copyright
Copyright © Springer-Verlag 2005

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