Speaker
Irene Tamborra
Description
Neutrinos are key particles in the core collapse of massive stars, crucially affecting the supernova inner workings. In addition, non-standard feebly interacting particles may be abundantly produced in the hot and dense supernova core, making the latter a unique laboratory to explore physic beyond the Standard Model. Fascinating recent developments on the physics of neutrinos and other weakly interacting particles in core-collapse supernovae will be reviewed.
