Measuring the atmospheric neutrino oscillation parameters and constraining the 3+1 neutrino model with ten years of ANTARES data

Abstract

The ANTARES neutrino telescope has an energy threshold of a few tens of GeV. This allows to study the phenomenon of atmospheric muon neutrino disappearance due to neutrino oscillations. In a similar way, constraints on the 3+1 neutrino model, which foresees the existence of one sterile neutrino, can be inferred. Using data collected by the ANTARES neutrino telescope from 2007 to 2016, a new measurement of $\Delta m_{32}^2$ and ${\theta }_{23}$ has been performed - which is consistent with world best-fit values - and constraints on the 3+1 neutrino model have been derived.

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Cited by in corpus (4)

• Model-Independent Constraints on Non-Unitary Neutrino Mixing from High-Precision Long-Baseline Experiments
• Probing Lorentz Invariance Violation with Atmospheric Neutrinos at INO-ICAL
• Evolution of Neutrino Mass-Mixing Parameters in Matter with Non-Standard Interactions
• Exploration of mass splitting and muon/tau mixing parameters for an eV-scale sterile neutrino with IceCube