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Low energy atmospheric muon neutrinos in MACRO
Journal article   Open access   Peer reviewed

Low energy atmospheric muon neutrinos in MACRO

M. Ambrosio, R. Antolini, G. Auriemma, D. Bakari, A. Baldini, G.C. Barbarino, B.C. Barish, G. Battistoni, R. Bellotti, C. Bemporad, …
Physics letters. B, v 478(1), pp 5-13
2000
url
https://doi.org/10.1016/s0370-2693(00)00267-7View
Published, Version of Record (VoR)Open Access (License Unspecified) Open
url
https://doi.org/10.1016/S0370-2693(00)00267-7View
Published, Version of Record (VoR) Open

Abstract

We present the measurement of two event samples induced by atmospheric ν μ of average energy E ν∼4 GeV. In the first sample, a neutrino interacts inside the MACRO detector producing an upward-going muon leaving the apparatus. The ratio of the number of observed to expected events is 0.57±0.05 stat±0.06 syst±0.14 theor with an angular distribution similar to that expected from the Bartol atmospheric neutrino flux. The second is a mixed sample of internally produced downward-going muons and externally produced upward-going muons stopping inside the detector. These two subsamples are selected by topological criteria; the lack of timing information makes it impossible to distinguish stopping from downgoing muons. The ratio of the number of observed to expected events is 0.71±0.05 stat±0.07 syst±0.18 theor. The observed deficits in each subsample is in agreement with neutrino oscillations, although the significance is reduced by the large theoretical errors. However, the ratio of the two samples causes a large cancellation of theoretical and of some systematic errors. With the ratio, we rule out the no-oscillation hypothesis at 95% c.l. Furthermore, the ratio tests the pathlength dependence of possible oscillations. The data of both samples and their ratio favor maximal mixing and Δm 2∼10 −3–10 −2 eV 2. These parameters are in agreement with our results from upward throughgoing muons, induced by ν μ of much higher energies.

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Domestic collaboration
International collaboration
Web of Science research areas
Astronomy & Astrophysics
Physics, Nuclear
Physics, Particles & Fields
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