OSCILLATION INVESTIGATIONS IN SOUDAN 2: ATMOSPHERIC νμ → ντ AND ${\rm n} \to \bar{n}$ IN IRON

2003 ◽  
Vol 18 (22) ◽  
pp. 3821-3840
Author(s):  
ANTHONY MANN ◽  
MAYLY SANCHEZ ◽  
TOMAS KAFKA

The 5.90 fiducial kiloton-year exposure of the Soudan-2 iron tracking calorimeter is analyzed for effects of neutrino oscillations. Using fully contained single track, single shower and multiprong events, we determine the atmospheric νμ/νe ratio-of-ratios in the sub-GeV Eν regime to be R=0.68±0.12±0.06. Assuming this anomalously low R-value to be the result of νμ flavor disappearance via νμ → ντ oscillation, we distribute fully contained and partially contained events into bins of log (L/Eν) and fit to oscillation hypotheses using extended maximum likelihood. The region in the ( sin 22θ, Δm2) plane allowed at 90% CL is obtained using the Feldman-Cousins procedure: 0.52< sin 2 2θ≤1.0 and 3×10-4<Δm2<2×10-2 eV 2. A different oscillation process which could occur in our contained event samples is baryon instability in the form of neutron-antineutron oscillations. Our search requires candidate [Formula: see text] occurrences to have ≥ 4 prongs (tracks and showers) and to have kinematics compatible with [Formula: see text] annihilation within a nucleus. We observe five candidate events, with estimated atmospheric neutrino plus cosmic ray backgrounds totalling 4.5 ± 1.2 events. Previous experiments with smaller exposures observed no candidates, with estimated background rates similar to this experiment. We set a lifetime lower limit at 90% CL for the [Formula: see text] oscillation time in iron: TA(Fe)>7.2×1031 years. The corresponding lower limit for oscillation of free neutrons is [Formula: see text] seconds.

2001 ◽  
Vol 16 (supp01b) ◽  
pp. 736-738
Author(s):  
◽  
FRANCESCO TERRANOVA

MONOLITH is a proposed massive (34 kton) magnetized tracking calorimeter at the Gran Sasso laboratory in Italy, optimized for the detection of high energy atmospheric muon neutrinos. The main goal is to establish (or reject) the neutrino oscillation hypothesis through an explicit observation of the full first oscillation swing. The Δm2 sensitivity range for this measurement comfortably covers the complete Super-Kamiokande allowed region. Other measurements include studies of matter effects and the up/down ratio of NC events, the study of cosmic ray muons in the multi-TeV range, and auxiliary measurements from the CERN to Gran Sasso neutrino beam.


2005 ◽  
Vol 20 (14) ◽  
pp. 3059-3061 ◽  
Author(s):  
◽  
CHRISTOPHER SMITH

The MINOS experiment is designed to search for neutrino oscillations. A neutrino beam from Fermilab is observed by the Near and Far detectors, separated by 735km. A comparison of the observed neutrino events at the two locations allows a measurement of the oscillation parameters to be made. Commissioning of the Near detector is underway and the Far detector is collecting cosmic ray and atmospheric neutrino data. Analysis of the atmospheric neutrino events has begun and neutrino, antineutrino event separation has been achieved. Data collection with the NuMI beam will begin in December 2004.


1994 ◽  
Vol 09 (02) ◽  
pp. 169-179 ◽  
Author(s):  
R. FOOT

We re-examine neutrino oscillations in exact parity models. Previously it was shown in a specific model that large neutrino mixing angles result. We show here that this is a general result of neutrino mixing in exact parity models provided that the neutrino mass matrix is real. In this case, the effects of neutrino mixing in exact parity models is such that the probability of a given weak eigenstate remaining in that eigenstate averages to less than half when averaged over many oscillations. This result is interesting in view of the accumulating evidence for a significant deficit in the number of solar neutrinos. It may also be of relevance to the atmospheric neutrino anomaly.


1984 ◽  
Vol 30 (1) ◽  
pp. 80-88 ◽  
Author(s):  
G. V. Dass ◽  
K. V. L. Sarma

2001 ◽  
Vol T93 (1) ◽  
pp. 26
Author(s):  
M. C. Gonzalez-Garcia

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