Nucleosynthesis in 2D core-collapse supernovae of 11.2 and 17.0 M ☉ progenitors: implications for Mo and Ru production

@article{Eichler2018NucleosynthesisI2,
  title={Nucleosynthesis in 2D core-collapse supernovae of 11.2 and 17.0 M ☉ progenitors: implications for Mo and Ru production},
  author={Marius Eichler and K. Z. Nakamura and Tomoya Takiwaki and Takami Kuroda and Kei Kotake and Matthias Hempel and Rub'en M. Cabez'on and Matthias Liebendorfer and F. Thielemann},
  journal={Journal of Physics G},
  year={2018},
  volume={45},
  pages={014001}
}
Core-collapse supernovae are the first polluters of heavy elements in the galactic history. As such, it is important to study the nuclear compositions of their ejecta, and understand their dependence on the progenitor structure (e.g., mass, compactness, metallicity). Here, we present a detailed nucleosynthesis study based on two long-term, two-dimensional core-collapse supernova simulations of a 11.2 Mlsubg⊙l/subg and a 17.0 Mlsubg⊙l/subg star. We find that in both models nuclei well beyond the… Expand
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TLDR
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