Speaker
Noshad Khosravi Largani
Description
I will discuss recent simulation results of neutrino-driven supernova explosions launched from a low-mass 9.6 solar mass iron-core progenitors of low metalicity. The supernova simulations are based on general relativistic neutrino radiation hydrodynamics in spherical symmetry featuring six-species Boltzmann neutrino transport and a complete set of neutrino opacities. Special emphasis is devoted to the treatment of the Urca processes at the mean-field level.
| Length of presentation requested | Oral presentation: 17 min + 3 min questions |
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| Please select a keyword related to your abstract | Stellar Models and Galactic Chemical Evolution |
