Speaker
Jorge Martin Camalich
(IFIC-Valencia)
Description
I will discuss recent progress on the understanding of the production of light dark matter in core-collapse supernova explosions. This leads to not only a constraint in the relevant parameter space due to cooling arguments of SN 1987A but also to a range of phenomenological consequences that can open new venues for detection. In particular, we will focus on the application to sub-GeV dark matter candidates
Author
Jorge Martin Camalich
(IFIC-Valencia)
