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Münster 2017 – wissenschaftliches Programm

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HK: Fachverband Physik der Hadronen und Kerne

HK 23: Nuclear Astrophysics II

HK 23.6: Vortrag

Dienstag, 28. März 2017, 15:30–15:45, F 33

Simulation of neutrino-driven winds from core-collapse supernovae — •Maximilian Witt1 and Almudena Arcones1,21Institut für Kernphysik, TU Darmstadt, Germany — 2GSI Helmholtzzentrum für Schwerionenforschung GmbH, Darmstadt, Germany

Neutrino-driven winds occur after core-collapse supernovae, when the hot proto-neutron star cools by radiating neutrinos. Within the continuous mass outflow that is ejected at supersonic velocities, heavy elements up to silver may form [1].

We have developed a steady-state model that was used to compare to our 1D and 2D hydrodynamic simulations. We have investigated the conditions which lead to a neutrino-driven wind and will discuss how this affects the nucleosynthesis in core-collapse supernovae.

[1] A. Arcones, F.-K. Thielemann, J.Phys. G 40 (2013) 013201

Supported by the Helmholtz-University Young Investigator grant No. VH-NG-825, the SFB 1245 and the ERC grant No. 677912 EUROPIUM.

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