Neutrino Propagation in Matter
arXiv:hep-ph/9808281 · doi:10.1016/S0370-1573(99)00017-4
Abstract
The enhancement of neutrino oscillations in matter is briefly reviewed. Exact and approximate solutions of the equations describing neutrino oscillations in matter are discussed. The role of stochasticity of the media that the neutrinos propagate through is elucidated.
17 pages, 5 figures. Expanded version of a talk at the Slansky Memorial Symposium, Los Alamos, May 1998
References in corpus (6)
- Where do we stand with solar neutrino oscillations?
- Diffractive-Like (or Parametric-Resonance-Like?) Enhancement of the Earth (Day-Night) Effect for Solar Neutrinos Crossing the Earth Core
- Algebraic Approach to Shape Invariance
- Variations on Four-Neutrino Oscillations
- Matter-Enhanced Neutrino Oscillations in the Quasi-Adiabatic Limit
- Exact Solutions for Matter-Enhanced Neutrino Oscillations
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- Supernova Neutrino-Nucleus Astrophysics
- Non-standard interactions and the CP phase measurements in neutrino oscillations at low energies
- Global Analysis of Solar Neutrino and KamLAND Data
- Magnetic Field Generation from Self-Consistent Collective Neutrino-Plasma Interactions
- Do the KamLAND and Solar Neutrino Data Rule out Solar Density Fluctuations?
- Probing the Sun's inner core using solar neutrinos: a new diagnostic method
- The Last Neutrino Mixing angle theta13
- Solar Neutrino Matter Effects Redux
- Inference finds consistency between a neutrino flavor evolution model and Earth-based solar neutrino measurements
- Neutrino Experiments and Their Implications
- Physics Potential of Solar Neutrino Experiments