Supernova constraints on dark flavored sectors
Proto-neutron stars forming a few seconds after core-collapse supernovae are hot and dense environments where hyperons can be efficiently produced by weak processes. By making use of various state-of-the-art supernova simulations combined with the proper extensions of the equations of state including Λ hyperons, we calculate the cooling of the star
Martin Camalich, Jorge et al.
Fecha de publicación:
6
2021