Collective Neutrino Oscillations
arXiv:1001.2799 · doi:10.1146/annurev.nucl.012809.104524
Abstract
We review the rich phenomena associated with neutrino flavor transformation in the presence of neutrino self-coupling. Our exposition centers on three collective neutrino oscillation scenarios: a simple bipolar neutrino system that initially consists of mono-energetic electron neutrinos and antineutrinos; a homogeneous and isotropic neutrino gas with multiple neutrino/antineutrino species and continuous energy spectra; and a generic neutrino gas in an anisotropic environment. We use each of these scenarios to illustrate key facets of collective neutrino oscillations. We discuss the implications of collective neutrino flavor oscillations for core collapse supernova physics and for the prospects of obtaining fundamental neutrino properties, e.g., the neutrino mass hierarchy and from a future observed supernova neutrino signal.
Submitted to Annual Review of Nuclear and Particle Science
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- Theoretical Results on Neutrinos
- Spin-Flavor Precession Phase Effects in Supernova
- Spin Flavor Spectral Splits of Supernova Neutrino Flavor Conversions
- Fast flavor conversion of neutrinos in presence of matter bulk velocity
- Non-Standard Neutrino Self-Interactions Can Cause Neutrino Flavor Equipartition Inside the Supernova Core
- Two-beam Multiparticle Many-body simulations of Inhomogeneous FFI
- Neutrino effective potential and damping in a fermion and scalar background in the resonance region
- Neutrino-(anti)neutrino forward scattering potential for massive neutrinos at low energies
- Testing common approximations of neutrino fast flavor conversion
- On Possibility of Determining Neutrino Mass Hierarchy by the Charged-Current and Neutral-Current Events of Supernova Neutrinos in Scintillation Detectors
- Single-wave solutions of the neutrino fast flavor system. Part I. Mechanical properties
- Neutrinos from Diffuse Supernova Background
- Nucleosynthesis: what direct reactions can do for it?
- Status and Perspectives of Neutrino Physics
- Where, when and why: occurrence of fast-pairwise collective neutrino oscillation in three-dimensional core-collapse supernova models
- Interactions of Neutrino Wave Packets
- Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes
- On the Independent Crossing Approximation in Three Flavor Neutrino Oscillations
- Supernova neutrino flavor evolution at high densities
- Neutrino oscillations in a trapping potential
- Towards First Detection of the Solar MSW Transition With JUNO
- Neutrino astrophysics and its connections to nuclear physics
- An Outlook on Nuclear Physics
- Inference of bipolar neutrino flavor oscillations near a core-collapse supernova, based on multiple measurements at Earth
- Fast Neutrino Conversion in Hydrodynamic Simulations of Neutrino-Cooled Accretion Disks
- Single-wave solutions of the neutrino fast flavor system. Part II. Weak instabilities and their resonant behavior
- Performance Analysis of an Astrophysical Simulation Code on the Intel Xeon Phi Architecture
- Simulating collective neutrinos oscillations on the Intel Many Integrated Core (MIC) architecture
- Neutrinos and core-collapse supernovae
- Symmetries of Neutrino Physics
- Nuclear Physics and Astrophysics of Neutrino Oscillations
- Oscillation-Independent Probes of Neutrino Non-Standard Interactions from Supernovae
- Neutrino quantum kinetics in three flavors
- Astrophysical Neutrinos and Flavor Evolution With Self Interaction
- Effects of spacetime geometry on neutrino oscillation inside a Core-Collapse Supernova
- Supernova Detection at SNOLAB
- Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities
- Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
- Accounting for the Heisenberg and Pauli principles in the kinetic approach to neutrino oscillations
- Neutrinos, Rare Isotopes of Exotic Nuclei and Nuclear Astrophysics
- Neutrino dispersion relation in a magnetized multi-stream matter background
- Supernova flavour conversions in DUNE: the slow, the fast and the standard
- Distinguishing Dirac and Majorana Neutrinos: Resonant Spin-Flavor Precession of GeV-Scale Astrophysical Transients