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On Fast Neutrino Flavor Conversion Modes in the Nonlinear Regime

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arxiv 1811.04215 v2 pith:PCDX2DOR submitted 2018-11-10 astro-ph.HE

classification astro-ph.HE
keywords fastflavormodesneutrinocollectiveconversionleadoscillations
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abstract

A dense neutrino medium could experience self-induced flavor conversions on relatively small scales in the presence of the so-called fast flavor conversion modes. Owing to the fact that fast conversion scales could be much smaller than the ones of the traditional collective neutrino oscillations, it has been speculated that fast modes could lead to some sort of flavor decoherence/equilibrium. We study the evolution of fast modes in the nonlinear regime and we show that not only fast modes are not guaranteed to lead to flavor equilibrium, but also they could lead to some sort of collective neutrino oscillations but on scales determined by neutrino number density. For the $\nu_e$ dominated case, we observe large amplitude collective oscillations, whereas a sort of flavor stabilization is reached for the $\bar{\nu}_e$ dominated case.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Tau lepton asymmetry by sterile neutrino emission -- Moving beyond one-zone supernova models

    astro-ph.HE 2019-08 conditional novelty 7.0 of 10

    keV-mass sterile neutrinos mixing with tau neutrinos can generate a tau lepton asymmetry larger than 0.15, and including the dynamical feedback relaxes supernova bounds on sterile neutrino mixing.

  2. Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Nearby neutrino flavor conversion in a supernova can boost νp-process yields of p-nuclides like 92Mo and 92Nb by up to two orders of magnitude, matching solar abundances when conversion starts within ~10 km of the pro...

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