Neutrinos self interactions in Supernovae

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dc.creatorFogli, Gianluigi
dc.creatorLisi, Eligio
dc.creatorMarrone, Antonio
dc.creatorMirizzi, Alessandro
dc.date2008-05-16
dc.date.accessioned2026-07-07T09:39:25Z
dc.date.available2026-07-07T09:39:25Z
dc.descriptionOscillations of neutrino emerging from a supernova core are studied. In this extremely high density region neutrino self interactions induce collective flavor transitions. When collective transitions are decoupled from matter oscillations, as for our chosen matter profile, an analytical interpretation of the collective effects is possible, by means of a mechanical analogy with a spherical pendulum. For inverted neutrino hierarchy the neutrino propagation can be divided in three regimes: synchronization, bipolar oscillations, and spectral split. Our simulation shows that averaging over neutrino trajectories does not alter the nature of these three regimes.
dc.description6 pages, 7 figures, to appear in the Proceedings of the 43rd Rencontres de Moriond EW session, La Thuile, Italy, 1-8 March 2008
dc.identifierhttps://arxiv.org/abs/0805.2530
dc.identifierhttp://arxiv.org/abs/0805.2530
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/161163
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrinos self interactions in Supernovae
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