Supernova neutrino flavor evolution at high densities
arXiv:1111.2282
Abstract
These conference proceedings cover various aspects of neutrino propagation through the high matter and neutrino densities near the proto-neutron star in a core-collapse supernova. A significant feature of this regime is the impact of neutrino-neutrino interactions. Properties of this non-linear many-neutrino system are discussed with a particular emphasis on its symmetries.
Proceedings of the "HAmburg neutrinos from Supernova Explosions (HANSE 2011)" workshop, DESY, Hamburg Site (Germany) from 19 to 23 July 2011
References in corpus (19)
- The multi-angle instability in dense neutrino systems
- Analysis of Collective Neutrino Flavor Transformation in Supernovae
- IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae
- Adiabaticity and spectral splits in collective neutrino transformations
- Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
- Collective neutrinos oscillation in matter and CP-violation
- Analysis of matter suppression in collective neutrino oscillations during the supernova accretion phase
- Spectral split in prompt supernova neutrino burst: Analytic three-flavor treatment
- Damping of supernova neutrino transitions in stochastic shock-wave density profiles
- Stepwise Spectral Swapping with Three Neutrino Flavors
- Impact of eV-mass sterile neutrinos on neutrino-driven supernova outflows
- Turbulence effects on supernova neutrinos
- Possible CP-Violation effects in core-collapse Supernovae
- Construction and analysis of a simplified many-body neutrino model
- Simulating nonlinear neutrino flavor evolution
- Instability in the dense supernova neutrino gas with flavor-dependent angular distributions
- Three Flavor Neutrino Oscillations in Matter: Flavor Diagonal Potentials, the Adiabatic Basis and the CP phase
- Neutrino Luminosity and Matter-Induced Modification of Collective Neutrino Flavor Oscillations in Supernovae
- Density Fluctuation Effects on Collective Neutrino Oscillations in O-Ne-Mg Core-Collapse Supernovae