PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Neutrino. NU-atmospheric neutrinos and neutrino properties
Sensitivity of the ANTARES neutrino telescope to atmospheric neutrino oscillation parameters
I. Salvadori*  on behalf of the ANTARES Collaboration
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
A new analysis, aimed at improving the current ANTARES measurement of the atmospheric neu-
trino oscillation parameters, is presented in these proceedings. Two different track reconstruction
procedures are combined in order to increase the sensitivity. Furthermore, a novel method to
estimate the neutrino energy is applied. A complete 3-flavour description of the oscillation prob-
ability including matter effects in the Earth is used. By performing a two-dimensional fit of the
event rate as a function of reconstructed energy and zenith angle, expectations on the sensitivity to
the oscillation parameters are derived. Using the same analysis chain, a study on the ANTARES
sensitivity to sterile neutrinos is performed.
DOI: https://doi.org/10.22323/1.301.1026
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