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

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arxiv 1812.08650 v3 pith:4UJMXYHK submitted 2018-12-20 hep-ex hep-ph

ANTARES Collaboration: A. Albert (1) , M. André (2) , M. Anghinolfi (3) , G. Anton (4) , M. Ardid (5) , J.-J. Aubert (6) , J. Aublin (7) , T. Avgitas (7)
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classification hep-exhep-ph
keywords neutrinoantaresmodelatmosphericbeenconstraintsdatatelescope
verification ladder T0 review T1 audit T2 compute T3 formal
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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 $\Delta m^2_{32}$ 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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