Exploding and non-exploding core-collapse supernova models in 3D and the multi-messenger analysis.

by Kei Kotake (Fukuoka University)

Monday 20 May 2019, 16:00 → 18:00 Europe/Rome

Aula Conversi (Dipartimento di Fisica - Ed. G. Marconi)

How massive stars end their lives has been a time-honored  riddle of astrophysics over the decades. Based on three-dimensional  radiation-hydrodynamics simulations, I report several new results of core-collapse supernova models, leading to a neutron-star and black-hole formation in the stellar centre. I will also discuss how one could extract the  information of the supernova engines by deciphering the multi-messenger observables particularly focusing on the gravitational-wave and neutrino emission.