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SYGP: Symposium Gemeinsame Probleme in Fusions- und astrophysikalischen Plasmen

SYGP 1: Invited Talks

SYGP 1.4: Hauptvortrag

Montag, 12. März 2012, 11:45–12:10, V55.22

The role of magnetic fields in core collapse supernovae — •Ewald Mueller — Max-Planck-Institut fuer Astrophysik, 85748 Garching, Deutschland

Simulations of core collapse supernovae pose a true challenge as they require a proper treatment of multi-dimensional neutrino radiation hydrodynamics, and possibly magneto-hydrodynamic processes. In my talk I will address the current status of core collapse supernova modeling, discuss magneto-hydrodynamic processes that can amplify a magnetic seed field during a core collapse supernova explosion, and present recent results from MHD core collapse simulations.