Elaborating the ultimate fate of fast collective neutrino flavor oscillations

Dense clouds of neutrinos and antineutrinos can exhibit fast collective flavor oscillations. Previously, in [S. Bhattacharyya and B. Dasgupta, Phys. Rev. Lett. 126, 061302 (2021).], we proposed that such flavor oscillations lead to depolarization—i.e., an irreversible mixing of the flavors—whose extent depends on the initial momentum distributions of the different flavors. In this paper, we elaborate and extend this proposal, and compare it with related results in the literature. We present an accurate analytical estimate for the lower resting point of the fast flavor pendulum and underline the relaxation mechanisms—i.e., transverse relaxation, multipole cascade, and mixing of flavor waves—that cause it to settle down. We estimate the extent of depolarization, its dependence on momentum and net lepton asymmetry, and its generalization to three flavors. Finally, we prescribe approximate analytical recipes for the depolarized distributions and fluxes that can be used in supernova/nucleosynthesis simulations and supernova neutrino phenomenology.

Note:

v3: Definitions of some quantities and a few extra sentences have been added in Section.II and Section.III for clarity purposes. Matches version published in PRD

neutrino: oscillation
flavor: oscillation
neutrino: flavor
neutrino: cloud
flavor: mixing
lepton: asymmetry
neutrino: supernova
collective
depolarization
multipole

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