Studying atmospheric neutrino oscillations in the few-GeV range with a
multimegaton 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.
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)