Speaker
Milad Delfan Azari
(Waseda University)
Description
In one of the most promising supernova theories, neutrino-heating mechanism, neutrinos carry the majority of the energy released during the gravitational collapse of massive stars. If neutrino flavors are converted fast in the cores, by depositing energy, they can rejuvenate stalled bounce shocks and provide the energy for supernova explosions. In this talk, I will present the results of our investigations on the dynamics of fast neutrino flavor conversions with collisions under energy-dependent treatment in detail, based on the results of self-consistent, realistic Boltzmann simulations of core-collapse supernovae in two spatial dimensions under axisymmetry.
| Please select a main topic related to your abstract | Explosive Stellar Objects and Nuclear Physics |
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Primary author
Milad Delfan Azari
(Waseda University)
Co-authors
Hirokazu Sasaki
(Los Alamos National Laboratory)
Tomoya Takiwaki
(National Astronomical Observatory of Japan)
Hirotada Okawa
(Waseda University)
Shoichi Yamada
(Waseda University)
