Core-collapse supernova simulations: Variations of the input physics

Details Core-collapse supernova simulations: Variations of the input physics Core-collapse supernova simulations: Variations of the input physics

2002-03-27

arxiv.org/abs/astro-ph/0203493v1

Astronomy and Astrophysics

Astrophysics

6 pages, 6 ps figures (in color), to appear in W. Hillebrandt and E. Mueller, eds., Proceedings of the 11th Workshop on "Nucle

Scientific paper

Spherically symmetric simulations of stellar core collapse and post-bounce evolution are used to test the sensitivity of the supernova dynamics to different variations of the input physics. We consider a state-of-the-art description of the neutrino-nucleon interactions, possible lepton-number changing neutrino reactions in the neutron star, and the potential impact of hydrodynamic mixing behind the supernova shock.

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