Speaker
Alina Vishneva
Description
About 1% of solar neutrinos are produced in the CNO cycle. Despite their subdominant role in the energy production, CNO neutrinos provide important information on the abundance of heavy elements in the solar core. In this work we present the details of the final analysis of Borexino data for measuring the flux of solar CNO neutrinos. This analysis features the fit of the electron recoil spectrum alongside with the directional information of neutrino events.
Primary author
Alina Vishneva
