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Nucleosynthesis in Multi-Dimensional Simulations of SNII
Published online by Cambridge University Press: 19 September 2016
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
- Copyright
- Copyright © Springer-Verlag 2005
References
4.
Kifonidis, K., Plewa, T., Janka, H.-Th., Müller, E.: Astrophys. J. Lett.
531
L123 (2000)Google Scholar
5.
Kifonidis, K., Plewa, T., Janka, H.-Th., Müller, E.: Astron. Astrophys.
408, 621 (2003)Google Scholar
7.
Maeda, K., Nakamura, T., Nomoto, K., Mazzali, P., Patat, F., Hachisu, I.: Astrophys. J.
565, 405 (1992)Google Scholar
8.
Nagataki, S., Hashimoto, M.-A., Sato, K., Yamada, S.: Astrophys. J.
486, 1026 (1997)Google Scholar
9.
Niemeyer, J., Reinecke, M., Travaglio, C., Hillebrandt, W. 2002: In Workshop From Twilight to Highlight: The Physics of Supernovae, p. 151Google Scholar
10.
Rauscher, T., Heger, A., Hoffman, R.D., Woosley, S.E.: Astrophys. J.
576
323 (2002)Google Scholar