Neutrinos and Symmetries
arXiv:0910.1814 · doi:10.1016/j.nuclphysa.2010.05.007
Abstract
Three facets of symmetries in neutrino physics are briefly reviewed: i) The SO(5) symmetry of the neutrino mass and and its connection to the see-saw mechanism; ii) Flavor SU(N) symmetries of dense, self-interacting neutrino gases in astrophysical settings; iii) The neutrino mixing angle theta13 and possible CP-violation in the neutrino sector.
5 pages of LATEX; to appear in the proceedings 4th International Symposium on Symmetries in Subatomic Physics held on June 2-5, 2009 at Department of Physics, National Taiwan University, Taipei, Taiwan
References in corpus (14)
- Collective neutrino flavor transitions in supernovae and the role of trajectory averaging
- Multiple Spectral Splits of Supernova Neutrinos
- Analysis of Collective Neutrino Flavor Transformation in Supernovae
- Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
- Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter
- Neutrino flavour transformation in supernovae
- Simple Picture for Neutrino Flavor Transformation in Supernovae
- Collective neutrinos oscillation in matter and CP-violation
- Possible CP-Violation effects in core-collapse Supernovae
- Contrasting solar and reactor neutrinos with a non-zero value of theta13
- Construction and analysis of a simplified many-body neutrino model
- Three Flavor Neutrino Oscillations in Matter: Flavor Diagonal Potentials, the Adiabatic Basis and the CP phase
- Symmetries in collective neutrino oscillations
- Implications of the Super-K atmospheric data for the mixing angles and
Cited by in corpus (6)
- Invariants of Collective Neutrino Oscillations
- Exact solution of multi-angle quantum many-body collective neutrino flavor oscillations
- Entanglement and correlations in fast collective neutrino flavor oscillations
- Neutrinos and rare isotopes
- Flavor Oscillations in Core-Collapse Supernovae
- Supernova neutrino flavor evolution at high densities