Flavor Oscillations in Core-Collapse Supernovae
arXiv:1209.5894 · doi:10.1016/j.nuclphysbps.2013.04.037
Abstract
Core collapse supernovae are unique laboratories to study many aspects of neutrino physics. The vicinity of the proto-neutron star in a core-collapse supernova is characterized by large matter and neutrino densities. A salient feature of this region is the impact of neutrino-neutrino interactions. Properties of the ensuing non-linear many-neutrino system are examined with a particular emphasis on its collective behavior and its symmetries. The impact of neutrino properties and interactions on the r-process nucleosynthesis that may take place in the supernova environment is discussed.
Talk at Neutrino 2012, Kyoto, Japan, June 3-9, 2012. 7 pages, one figure
References in corpus (26)
- The Reactor Antineutrino Anomaly
- Collective neutrino flavor transitions in supernovae and the role of trajectory averaging
- The Diffuse Supernova Neutrino Background
- Multiple Spectral Splits of Supernova Neutrinos
- The multi-angle instability in dense neutrino systems
- Analysis of Collective Neutrino Flavor Transformation in Supernovae
- Adiabaticity and spectral splits in collective neutrino transformations
- Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
- Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter
- Neutrino scattering and flavor transformation in supernovae
- Implications of 3+1 Short-Baseline Neutrino Oscillations
- Analysis of matter suppression in collective neutrino oscillations during the supernova accretion phase
- Collective neutrinos oscillation in matter and CP-violation
- Impact of eV-mass sterile neutrinos on neutrino-driven supernova outflows
- Sterile Neutrino-Enhanced Supernova Explosions
- Turbulence effects on supernova neutrinos
- Testing the very-short-baseline neutrino anomalies at the solar sector
- Possible CP-Violation effects in core-collapse Supernovae
- Construction and analysis of a simplified many-body neutrino model
- Stability analysis of collective neutrino oscillations in the supernova accretion phase with realistic energy and angle distributions
- 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
- Multi-Angle Simulation of Flavor Evolution in the Neutrino Neutronization Burst From an O-Ne-Mg Core-Collapse Supernova
- Symmetries in collective neutrino oscillations
- Density Fluctuation Effects on Collective Neutrino Oscillations in O-Ne-Mg Core-Collapse Supernovae
- Solar Neutrino Matter Effects Redux