Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously
occurs iin core-collapse supernovae and binary neutron star mergers, the lack of global …

The question of what ingredients characterize the quasisteady state of fast neutrino-flavor
conversion (FFC) is one of the longstanding riddles in neutrino oscillation. Addressing this …

We examine the effect of neutrino flavor transformation by the fast flavor instability (FFI) on
long-term mass ejection from accretion disks formed after neutron star mergers. Neutrino …

Neutrino flavor instabilities have the potential to shuffle neutrinos between electron, mu, and
tau flavor states, possibly modifying the core-collapse supernova mechanism and the heavy …

The fast flavor instability (FFI) is expected to be ubiquitous in core-collapse supernovae and
neutron star mergers. It rapidly shuffles neutrino flavor in a way that could impact the …

The neutrino fast flavor instability (FFI) can change neutrino flavor on time scales of
nanoseconds and length scales of centimeters. It is expected to be ubiquitous in core …

The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a
critically important unsolved problem in astrophysics. Following the electron flavor evolution …

We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale
and large-scale numerical simulations in spherical symmetry. We find that FFCs can, in …

We developed a new general-relativistic quantum-kinetics neutrino transport code,
GRQKNT, for numerical studies of quantum kinetics of nonequilibrium neutrinos in six …

Neutrinos propagating in dense neutrino media such as core-collapse supernovae and
neutron star merger remnants can experience the so-called fast flavor conversions on scales …