Jul 5 – 10, 2021
Europe/Rome timezone

Electron neutrino survival probability in the energy range: 5 keV- 15 MeV

Jul 6, 2021, 6:55 AM
Invited talk in the parallel session Why and how the Sun and the Stars shine: the Borexino experiment Why and How the Sun and the Stars Shine: the Borexino Experiment


Marco Pallavicini (INFN and University of Genova)


Solar neutrinos provide a sample of electron neutrinos of different energies. They are therefore a unique probe of the electron neutrino propagation through solar matter and for the experimental study of the MSW effect. Borexino, with its unique purity and sensitivity, has been able to study individually all components, extracting the best test of electron neutrino survival probability to date. The talk with summarise the results and the state of the art in the field.

Primary author

Marco Pallavicini (INFN and University of Genova)

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