Mass Hierarchy Determination via future Atmospheric Neutrino Detectors

Abstract

We study the problem of determination of the sign of Delta m^2_{31}, or the neutrino mass hierarchy, through observations of atmospheric neutrinos in future detectors. We consider two proposed detector types : (a) Megaton sized water Cerenkov detectors, which can measure the survival rates of nu_μ+ \barν_μand nu_e + \barν_e and (b) 100 kton sized magnetized iron detectors, which can measure the survival rates of ν_μand \barν_μ. For energies and path-lengths relevant to atmospheric neutrinos, these rates obtain significant matter contributions from P_{μe}, P_{μμ} and P_{ee}, leading to an appreciable sensitivity to the hierarchy. We do a binned χ^2 analysis of simulated data in these two types of detectors which includes the effect of smearing in neutrino energy and direction and incorporates detector efficiencies and relevant statistical, theoretical and systematic errors. We also marginalize the χ^2 over the allowed ranges of neutrino parameters in order to accurately account for their uncertainties. Finally, we compare the performance of both types of detectors vis a vis the hierarchy determination.

36 pages, 13 figures, revised version accepted in Physical Review D

References in corpus (1)

• Resolving parameter degeneracies in long-baseline experiments by atmospheric neutrino data

Cited by in corpus (4)

• Testing non-unitarity of neutrino mixing matrices at neutrino factories
• Identifying neutrino mass hierarchy at extremely small theta(13) through Earth matter effects in a supernova signal
• Neutrino mass hierarchy extraction using atmospheric neutrinos in ice
• Resolving the Mass Hierarchy with Atmospheric Neutrinos using a Liquid Argon Detector