Centre Tecnològic de Vilanova i la Geltrú
Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
2017-05-01
Studying atmospheric neutrino oscillations in the few-GeV range with a multi-megaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA water Cherenkov detector in the Mediterranean Sea. In this paper, the processes that limit the obtainable resolution in both energy and direction in charged-current neutrino events in the ORCA detector are investigated. These processes include the composition of the hadronic fragmentation products, the subsequent particle propagation and the photon-sampling fraction of the detector. GEANT simulations of neutrino interactions in seawater produced by GENIE are used to study the effects in the 1-20 GeV range. It is found that fluctuations in the hadronic cascade in conjunction with the variation of the inelasticity y are most detrimental to the resolutions. The effect of limited photon sampling in the detector is of significantly less importance. These results will therefore also be applicable to similar detectors/media, such as those in ice.
Postprint (author's final draft)
Article
Anglès
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica; Neutrinos; Neutrino astrophysics; Astronomy--Observations; Neutrino Detectors and Telescopes (experiments); Neutrins; Astrofísica
https://link.springer.com/article/10.1007%2FJHEP05%282017%29008
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
Open Access
Attribution-NonCommercial-NoDerivs 3.0 Spain
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