%0 Journal Article
%T Measuring the atmospheric neutrino oscillation parameters and constraining the 3+1 neutrino model with ten years of ANTARES data
%A ANTARES Collaboration (Albert, A. et al
%A Barrios-Marti, J.
%A Coleiro, A.
%A Colomer, M.
%A Gozzini, R.
%A Hernandez-Rey, J. J.
%A Illuminati, G.
%A Khan-Chowdhury, N. R.
%A Lotze, M.
%A Thakore, T.
%A Zornoza, J. D.
%A Zuñiga, J.
%J Journal of High Energy Physics
%D 2019
%V 06
%N 6
%I Springer
%@ 1029-8479
%G English
%F ANTARESCollaborationAlbert_etal2019
%O WOS:000472922700002
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=4066), last updated on Wed, 10 Jul 2019 08:57:18 +0000
%X 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 m 2 and (23) has been performed which is consistent with world best-fit values and constraints on the 3+1 neutrino model have been derived.
%K Neutrino Detectors and Telescopes (experiments)
%K Oscillation
%R 10.1007/JHEP06(2019)113
%U https://arxiv.org/abs/1812.08650
%U https://doi.org/10.1007/JHEP06(2019)113
%P 113-23pp