S E M I N A R I

Departament d'Astronomia i Astrofísica
Universitat de València

    Multi-D Core-Collapse Supernova Models: where we are and where we are going?

Kei Kotake

Department of Applied Physics, Fukuoka University, Japan


Seminari d'Astronomia i Astrofisica

Dimecres 25 març 2015

12:00


Resum

After we summarize a recent status of core-collapse supernova models, we report our recent results based on two-(2D) and three-dimensional (3D) radiation-hydrodynamics simulations. We also talk about signals of neutrinos and gravitational waves expected from the self-consistent models, which would be important to extract the information of the central engine from the multi-messenger observations. We also report our code development where 3D general-relativistic hydrodynamics is now meeting with spectral neutrino transport.