Volume 337 - Neutrino Oscillation Workshop (NOW2018) - Session III: Multimessenger astrophysics
Distinguishing SNν equalization from a pure MSW
F. Capozzi,* B. Dasgupta, A. Mirizzi
*corresponding author
Full text: pdf
Published on: April 24, 2019
Abstract
Among the theoretically possible flavor conversion scenarios of supernova neutrinos there are flavour equalization and the well known Mikheyev-Smirnov-Wolfenstein effect. We present a simple method to distinguish experimentally between them, using the combination of three detection channels: charged-current neutrino interaction on Argon, neutrino elastic scattering on protons and inverse $\beta$ decay.
DOI: https://doi.org/10.22323/1.337.0049
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