Neutrino–neutrino refraction dominates the flavor evolution in core-collapse supernovae,
neutron star mergers, and the early Universe. Ordinary neutrino flavor conversions develop …

We explore the impact of small-scale flavor conversions of neutrinos, the so-called fast flavor
conversions (FFCs), on the dynamical evolution and neutrino emission of core-collapse …

Fast and collisional flavor instabilities possibly occur in the neutrino decoupling regions of
core-collapse supernovae and neutron-star mergers. To gain a better understanding of the …

In compact astrophysical objects, the neutrino density can be so high that neutrino-neutrino
refraction can lead to fast flavor conversion of the kind ν e ν¯ e↔ ν x ν¯ x with x= μ, τ …

Flavor-dependent neutrino emission is critical to the evolution of a supernova and its
neutrino signal. In the dense anisotropic interior of the star, neutrino-neutrino forward …

In core-collapse supernovae or compact binary merger remnants, neutrino-neutrino
refraction can spawn fast pair conversion of the type ν e ν¯ e↔ ν x ν¯ x (with x= μ, τ) …

We present results from a self-consistent, non-rotating core-collapse supernova simulation
in three spatial dimensions using a binary evolution progenitor model of SN 1987A. This …

Recent theoretical work indicates that the neutrino radiation in core-collapse supernovae
may be susceptible to flavor instabilities that set in far behind the shock, grow extremely …

It has been speculated for a long time that neutrinos from a supernova (SN) may undergo
fast flavor conversions near the collapsed stellar core. We perform a detailed study of this …

At high densities in compact astrophysical sources, the coherent forward scattering of
neutrinos onto each other is responsible for making the flavor evolution nonlinear. Under the …