Understanding neutrino flavor transformation in dense environments such as core-collapse supernovae (CCSN) is critical for inferring nucleosynthesis and interpreting a detected neutrino signal. The role of direction-changing collisions in shaping the neutrino flavor field in these environments is important and poorly understood; it has not been treated self-consistently. There has been progress, via numerical integration, to include the effects of collisions in the dynamics of the neutrino flavor field. While this has led to important insights, integration is limited by its requirement that full initial conditions must be assumed known. On the contrary, feedback from collisions to the neutrino field is a boundary value problem. Numerical in...
Calibrating with detailed 2D core-collapse supernova simulations, we derive a simple core-collapse s...
The depth of our theoretical understanding of neutrino flavor mixing should match the importance of ...
Neutrinos are known to play important roles in many astrophysical scenarios from the early period of...
One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino fla...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
Neutrinos in compact-object environments, such as core-collapse supernovae, can experience various k...
We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and lar...
In core-collapse supernovae or compact binary merger remnants, neutrino-neutrino refraction can spaw...
Neutrino self-interactions in a dense neutrino gas can induce collective neutrino flavor conversions...
We discuss a new kind of astrophysical transport problem: the coherent evolution of neutrino flavor ...
The successful transition from core-collapse supernova simulations using classical neutrino transpor...
We calculate fast conversions of two flavor neutrinos by considering Boltzmann collisions of neutrin...
Neutrino propagation through a turbulent medium can be highly non-adiabatic leading to distinct sign...
The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a critical...
Recent multi-dimensional (multi-D) core-collapse supernova (CCSN) simulations characterize gravitati...
Calibrating with detailed 2D core-collapse supernova simulations, we derive a simple core-collapse s...
The depth of our theoretical understanding of neutrino flavor mixing should match the importance of ...
Neutrinos are known to play important roles in many astrophysical scenarios from the early period of...
One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino fla...
One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) ...
Neutrinos in compact-object environments, such as core-collapse supernovae, can experience various k...
We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and lar...
In core-collapse supernovae or compact binary merger remnants, neutrino-neutrino refraction can spaw...
Neutrino self-interactions in a dense neutrino gas can induce collective neutrino flavor conversions...
We discuss a new kind of astrophysical transport problem: the coherent evolution of neutrino flavor ...
The successful transition from core-collapse supernova simulations using classical neutrino transpor...
We calculate fast conversions of two flavor neutrinos by considering Boltzmann collisions of neutrin...
Neutrino propagation through a turbulent medium can be highly non-adiabatic leading to distinct sign...
The flavor evolution of neutrinos in core collapse supernovae and neutron star mergers is a critical...
Recent multi-dimensional (multi-D) core-collapse supernova (CCSN) simulations characterize gravitati...
Calibrating with detailed 2D core-collapse supernova simulations, we derive a simple core-collapse s...
The depth of our theoretical understanding of neutrino flavor mixing should match the importance of ...
Neutrinos are known to play important roles in many astrophysical scenarios from the early period of...