Collective flavor conversion in dense neutrino plasmas
hep-ph, astro-ph.CO, astro-ph.HE
Submitted: 2026-09-16
Updated: 2026-09-16
Comments: Contribution to Encyclopedia of Nuclear Physics
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Collective flavor conversions are interactions of neutrinos with quantized flavor waves
- New Developments in Flavor Evolution of a Dense Neutrino Gas
- Neutrinos from dense environments : Flavor mechanisms, theoretical approaches, observations, and new directions
- Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers
- Neutrinos from core-collapse supernovae
- Neutrino Quantum Kinetics
- A New Spin on Neutrino Quantum Kinetics
- Quantum transport theory for neutrinos with flavor and particle-antiparticle mixing
- Extended evolution equations for neutrino propagation in astrophysical and cosmological environments
- Neutrino-antineutrino correlations in dense anisotropic media
- Neutrino decoupling including flavour oscillations and primordial nucleosynthesis
- Inhomogeneous Kinetic Equation for Mixed Neutrinos: Tracing the Missing Energy
- Collective neutrino-antineutrino oscillations in dense neutrino environments?
- Neutrino propagation in media: Flavor-, helicity-, and pair correlations
- Theory of neutrino fast flavor evolution. Part I. Linear response theory and stability conditions
- Theory of neutrino fast flavor evolution. Part II. Solutions at the edge of instability
- Theory of neutrino slow flavor evolution. Part I. Homogeneous medium
- Theory of neutrino slow flavor evolution. Part II. Space-time evolution of linear instabilities
- Dispersion relation of the neutrino plasma: Unifying fast, slow, and collisional instabilities
- Lepton number crossings are insufficient for flavor instabilities
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