Neutrino self-interactions in a dense neutrino gas can induce collective neutrino flavor conversions. Fast neutrino flavor conversions (FFCs), one of the collective neutrino conversion modes, potentially change the dynamics and observables in core-collapse supernovae and binary neutron star mergers. In cases without neutrino-matter interactions (or collisions), FFCs are essentially energy-independent, and therefore the single energy treatment has been used in previous studies. However, neutrino-matter collisions in general depend on neutrino energy, suggesting that energy-dependent features may emerge in FFCs with collisions. In this paper, we perform dynamical simulations of FFCs with iso-energetic scatterings (emulating nucleon scattering...
Fast flavor conversions of supernova neutrinos, possible near the neutrinosphere, depends on an inte...
The core-collapse of massive stars and merger of neutron star binaries are among the most promising ...
Fast flavor conversions of supernova neutrinos, possible near the neutrinosphere, depends on an inte...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and lar...
We calculate fast conversions of two flavor neutrinos by considering Boltzmann collisions of neutrin...
Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs in...
The neutrino fast flavor instability (FFI) can change neutrino flavor on time scales of nanoseconds ...
Investigations on the resonance in the collisional flavor instability (CFI) of neutrinos, which were...
One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino fla...
In the dense supernova environment, neutrinos can undergo fast flavor conversions which depend on th...
Collective neutrino oscillations are critical to determine the neutrino flavor content, which has st...
The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a critical...
In core-collapse supernovae or compact binary merger remnants, neutrino-neutrino refraction can spaw...
Understanding neutrino flavor transformation in dense environments such as core-collapse supernovae ...
Fast flavor conversions of supernova neutrinos, possible near the neutrinosphere, depends on an inte...
The core-collapse of massive stars and merger of neutron star binaries are among the most promising ...
Fast flavor conversions of supernova neutrinos, possible near the neutrinosphere, depends on an inte...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and lar...
We calculate fast conversions of two flavor neutrinos by considering Boltzmann collisions of neutrin...
Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs in...
The neutrino fast flavor instability (FFI) can change neutrino flavor on time scales of nanoseconds ...
Investigations on the resonance in the collisional flavor instability (CFI) of neutrinos, which were...
One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino fla...
In the dense supernova environment, neutrinos can undergo fast flavor conversions which depend on th...
Collective neutrino oscillations are critical to determine the neutrino flavor content, which has st...
The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a critical...
In core-collapse supernovae or compact binary merger remnants, neutrino-neutrino refraction can spaw...
Understanding neutrino flavor transformation in dense environments such as core-collapse supernovae ...
Fast flavor conversions of supernova neutrinos, possible near the neutrinosphere, depends on an inte...
The core-collapse of massive stars and merger of neutron star binaries are among the most promising ...
Fast flavor conversions of supernova neutrinos, possible near the neutrinosphere, depends on an inte...