Relatore
Ko Nakamura
(Fukuoka University)
Descrizione
Systematic studies of core-collapse supernovae (CCSNe) have been conducted based on hundreds of one-dimensional artificial models (O'Connor & Ott 2011,2013; Ugliano et al. 2013, Ertl et al. 2015) and two-dimensional self-consistent simulations (Nakamura et al. 2015;2019, Burrows & Vartanyan 2020). We have performed three-dimensional magnetohydrodynamic simulations for the core-collapse of 16 progenitor models covering ZAMS mass between 9 and 24 solar masses. Our CCSN models show a wide variety of shock evolution, explosion energy, as well as multi-messenger signals including neutrinos. We present the dependence of the neutrino properties on the progenitor structure.
| Poster prize | No |
|---|---|
| Given name | Ko |
| Surname | Nakamura |
| First affiliation | Fukuoka University |
| Institutional email | nakamurako@fukuoka-u.ac.jp |
| Gender | Male |
Autore principale
Ko Nakamura
(Fukuoka University)
Coautore
Prof.
Jin Matsumoto
(Fukuoka University)
Prof.
Kei Kotake
(Fukuoka University)
Prof.
Tomoya Takiwaki
(NAOJ)
