Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1844959 | Nuclear Physics B - Proceedings Supplements | 2009 | 6 Pages |
Abstract
The potential of future high statistics atmospheric neutrino experiments is considered, having in mind currently discussed huge detectors of various technologies (water Cerekov, magnetized iron, liquid Argon). I focus on the possibility to use atmospheric data to determine the octant of θ23 and the neutrino mass hierarchy. The sensitivity to the θ23-octant of atmospheric neutrinos is competitive (or even superior) to long-baseline experiments. I discuss the ideal properties of a fictitious atmospheric neutrino detector to determine the neutrino mass hierarchy.
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