Solar Atmospheric Neutrinos searches with ANTARES neutrino telescope

Discussion timeslot (ZOOM-Meeting): 16. July 2021 - 12:00
ZOOM-Meeting URL: https://desy.zoom.us/j/91999581729
ZOOM-Meeting ID: 91999581729
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/36-Shower-Reconstruction-and-Pointing-NU/121
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-05/6

Abstract:
'The interaction of cosmic-rays with the solar atmosphere can yield neutrinos as final staternparticles. These neutrinos are expected to be mainly produced at the surface of the Sun and to bernabsorbed in the inner part.rnSolar Atmospheric Neutrinosu200b u200b represent an irreducible source of background to solar darkrnmatter searches, and its detection would be important in the characterization of thernbackground.rnThe deep-sea neutrino telescope ANTARES, located in the Mediterranean Sea, is well suited tornperform this search. In this work, 11 years of ANTARES data have been analysed and thernresulting sensitivities are presented.'

Authors: Daniel Lopez-Coto
Co-Authors: Sergio Navas | Juande Zornoza | for the ANTARES collaboration
Collaboration: AntaresKM3NeT

Indico-ID: 534
Proceeding URL: https://pos.sissa.it/395/1122