2 research outputs found

    The neutrino spectral split in core-collapse supernovae: a magnetic resonance phenomenon

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    A variety of neutrino flavour conversion phenomena occur in core-collapse supernova, due to the large neutrino density close to the neutrinosphere, and the importance of the neutrino-neutrino interaction. Three different regimes have been identified so far, usually called the synchronization, the bipolar oscillations and the spectral split. Using the formalism of polarization vectors, within two-flavours, we focus on the spectral split phenomenon and we show for the first time that the physical mechanism underlying the neutrino spectral split is a magnetic resonance phenomenon. In particular, we show that the precession frequencies fulfill the magnetic resonance conditions. Our numerical calculations show that the neutrino energies and the location at which the resonance takes place in the supernova coincide well with the neutrino energies at which a spectral swap occurs. The corresponding adiabaticity parameters present spikes at the resonance location.Comment: 11 pages, 9 figures, text and references adde

    Shockwaves in Supernovae: New Implications on the Diffuse Supernova Neutrino Background

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    We investigate shock wave effects upon the diffuse supernova neutrino background using dynamic profiles taken from hydrodynamical simulations and calculating the neutrino evolution in three flavors with the S-matrix formalism. We show that the shock wave impact is significant and introduces modifications of the relic fluxes by about 20%20 \% and of the associated event rates at the level of 1020%10-20 \%. Such an effect is important since it is of the same order as the rate variation introduced when different oscillation scenarios (i.e. hierarchy or θ13\theta_{13}) are considered. In addition, due to the shock wave, the rates become less sensitive to collective effects, in the inverted hierarchy and when sin22θ13\sin^2 2 \theta_{13} is between the Chooz limit and 10510^{-5}. We propose a simplified model to account for shock wave effects in future predictions.Comment: 8 pages, 9 figure
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