How collective modes terminate in the dispersion relation of neutrino plasmas
hep-ph, astro-ph.CO, astro-ph.HE
Submitted: 2026-09-29
Updated: 2026-09-29
Terminology
Sources
- 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
- Collective flavor conversion in dense neutrino plasmas
- Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion-Relation Approach
- Fast flavor conversions of supernova neutrinos: Classifying instabilities via dispersion relations
- Normal-mode Analysis for Collective Neutrino Oscillations
- The dispersion relation of the fast neutrino oscillation wave
- Theory of neutrino fast flavor evolution. Part I. Linear response theory and stability conditions
- Fast Flavor Pendulum: Instability Condition
- Dispersion relation of the neutrino plasma: Unifying fast, slow, and collisional instabilities
- 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
- Collective flavor conversions are interactions of neutrinos with quantized flavor waves
- Dynamic fast flavor oscillation waves in dense neutrino gases
- Fast Flavor Depolarization of Supernova Neutrinos
- Particle-in-cell Simulation of the Neutrino Fast Flavor Instability
- Collective fast neutrino flavor conversions in a 1D box: Initial condition and long-term evolution
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