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How collective modes terminate in the dispersion relation of neutrino plasmas
cosmology-and-nongalactic-astrophysicshigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenology
Neutrino plasmas support flavor waves, collective oscillations of flavor, that neutrinos can resonantly emit or absorb when they fulfill the Cherenkov condition. For massless neutrinos, this condition leads to singular features in the dispersion relation: Landau-damped modes, for example, disappear
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