Speaker
Jost Migenda
(University of Sheffield)
Description
This talk presents results of a study using Hyper-Kamiokande (HK) to distinguish different supernova models. With $\mathcal{O}(10^5)$ events expected in HK from a supernova near the galactic centre, such a model comparison will allow us to go beyond a simple determination of parameters of the neutrino flux, and to verify assumptions going into current supernova models.
Primary author
Jost Migenda
(University of Sheffield)
