Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016) 2017
DOI: 10.7566/jpscp.14.020604
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Nucleosynthesis in 2D Core-Collapse Supernova Long-Term Simulations of 11.2 and 17.0 \(\text{M}_{ \odot }\) Progenitors

Abstract: We perform detailed nucleosynthesis calculations for two long-term, 2D simulations of core-collapse supernovae. We find that elements are produced up to Ru (Z = 44) and observe abundance patterns that are characteristic of a νp-process. One important characteristic of the long-term simulation is that there is still accretion of matter onto the proto-neutron star and unbinding of matter in some other regions at the time when the simulations stop (around 7s). Dividing the tracer particles into different bins acc… Show more

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