  The study of neutrino flavour oscillations in astrophysical sources has been
boosted in the last two decades thanks to achievements in experimental neutrino
physics and observational astronomy. We here discuss two cases of interest in
the modelling of short and long gamma-ray bursts (GRBs): hypercritical, i.e.
highly super-Eddington spherical/disk accretion onto a neutron star (NS)/black
hole (BH). We show that in both systems the ambient conditions of density and
temperature imply the occurrence of neutrino flavour oscillations, with a
relevant role of neutrino self-interactions.
