2 research outputs found
The neutrino spectral split in core-collapse supernovae: a magnetic resonance phenomenon
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
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 and of the associated event
rates at the level of . 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 ) are considered. In addition, due to
the shock wave, the rates become less sensitive to collective effects, in the
inverted hierarchy and when is between the Chooz limit
and . We propose a simplified model to account for shock wave effects
in future predictions.Comment: 8 pages, 9 figure