Nucleosynthesis in 2D Core-Collapse Supernova Long-Term Simulations of 11.2 and 17.0 M⊙ Progenitors

Eichler, Marius and Nakamura, Ko and Takiwaki, Tomoya and Kuroda, Takami and Kotake, Kei and Hempel, Matthias and Cabezon, Ruben and Liebendörfer, Matthias and Thielemann, Friedrich-Karl. (2017) Nucleosynthesis in 2D Core-Collapse Supernova Long-Term Simulations of 11.2 and 17.0 M⊙ Progenitors. In: Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016), 14.

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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 according to their peak temperatures enables us to study and compare the nuclear compositions of these bins for the different simulations.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Astrophysik (Liebendörfer)
05 Faculty of Science > Departement Physik > Physik > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Hempel, Matthias
Item Type:Conference or Workshop Item, refereed
Conference or workshop item Subtype:Conference Paper
Publisher:Physical Society of Japan
Series Name:JPS Conference Proceedings
Note:Publication type according to Uni Basel Research Database: Conference paper
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Last Modified:12 Mar 2018 12:08
Deposited On:28 Dec 2017 08:05

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