579 research outputs found
A new ordering principle for the classical statistical analysis of Poisson processes with background
Inspired by the recent proposal by Feldman and Cousins of a ``unified
approach to the classical statistical analysis of small signals'' based on a
choice of ordering in Neyman's construction of classical confidence intervals,
I propose a new ordering principle for the classical statistical analysis of
Poisson processes with background which minimizes the effect on the resulting
confidence intervals of the observation of less background events than
expected. The new ordering principle is applied to the calculation of the
confidence region implied by the recent null result of the KARMEN neutrino
oscillation experiment.Comment: 16 pages including 5 figures, RevTeX. Final version published in
Phys. Rev. D 59 (1999) 05300
A High Statistics Search for Electron-Neutrino --> Tau-Neutrino Oscillations
We present new limits on nu_e to nu_tau and nu_e to nu_sterile oscillations
by searching for electron neutrino dissappearance in the high-energy wide-band
CCFR neutrino beam. Sensitivity to nu_tau appearance comes from tau decay modes
in which a large fraction of the energy deposited is electromagnetic. The beam
is composed primarily of muon neutrinos but this analysis uses the 2.3%
electron neutrino component of the beam. Electron neutrino energies range from
30 to 600 GeV and flight lengths vary from 0.9 to 1.4 km. This limit improves
the sensitivity of existing limits and obtains a lowest 90% confidence upper
limit in sin**2(2*alpha) of 9.9 x 10**(-2) at delta-m**2 of 125 eV**2.Comment: submitted to Phys. Rev. D. Rapid Com
Statistical Analysis of Different Muon-antineutrino->Electron-antineutrino Searches
A combined statistical analysis of the experimental results of the LSND and
KARMEN \numubnueb oscillation search is presented. LSND has evidence for
neutrino oscillations that is not confirmed by the KARMEN experiment. This
joint analysis is based on the final likelihood results for both data sets. A
frequentist approach is applied to deduce confidence regions. At a combined
confidence level of 36%, there is no area of oscillation parameters compatible
with both experiments. For the complementary confidence of 1-0.36=64%, there
are two well defined regions of oscillation parameters (sin^2(2th),Dm^2)
compatible with both experiments.Comment: 25 pages, including 10 figures, submitted to Phys. Rev.
Lepton Mixing Matrix in Standard Model Extended by One Sterile Neutrino
We consider the simplest extension of the standard electroweak model by one
sterile neutrino that allows for neutrino masses and mixing. We find that its
leptonic sector contains much less free physical parameters than previously
realized. In addition to the two neutrino masses, the lepton mixing matrix in
charged current interactions involves (n-1) free physical mixing angles for n
generations. The mixing matrix in neutral current interactions of neutrinos is
completely fixed by the two masses. Both interactions conserve CP. We
illustrate the phenomenological implications of the model by vacuum neutrino
oscillations, tritium beta decay and neutrinoless double beta decay. It turns
out that, due to the revealed specific structure in its mixing matrix, the
model with any n generations cannot accommodate simultaneously the data by
KamLAND, K2K and CHOOZ.Comment: 14 pages, no figures; version 2: (1) added a short paragraph at the
end of subsec 2.2 to record the counting of physical parameters for any
numbers of generations and sterile neutrinos for completeness; (2) added a
note in ref list, item [18] to quote and comment on an earlier work; (3)
added the second paper to ref list, item [17]; (4) fixed typo
New interactions in neutrino oscillations with three light flavors
If one assumes solar and LSND neutrino oscillations to explain the
corresponding data, then the atmospheric neutrino deficit cannot be
accommodated within the Standard Model with three light flavors, unless one
ignores the data's zenith-angle dependence. We propose a novel solution to this
problem by postulating large anomalous diagonal -quark interactions
which affect oscillations traversing the Earth and induce
the observed zenith-angle dependence.Comment: Final version, to appear in Phys. Rev. Letters dated May 25, 199
A Search for Muon-neutrino to Electron-neutrino and Muon-antineutrino to Electron-antineutrino Oscillations at NuTeV
Limits on and oscillations
are extracted using the NuTeV detector with sign-selected and
\nub_\mu beams. In \nub_\mu mode, for the case of ,
is excluded, and for
, . The NuTeV data exclude the
high end of oscillations parameters
favored by the LSND experiment without the need to assume that the oscillation
parameters for and \nub are the same. We present the most stringent
experimental limits for
oscillations in the large region.Comment: 4 pages, 3 figures. Submitted to Phys. Rev. Letters, UR-164
Constraints on Exotic Mixing of Three Neutrinos
Exotic explanations are considered for atmospheric neutrino observations. Our
analysis includes matter effects and the mixing of all three neutrinos under
the simplifying assumption of only one relevant mixing scale. Constraints from
accelerator, reactor and solar neutrinos are included. We find that the
proposed mixing mechanisms based on violations of Lorentz invariance or on
violations of the equivalence principle cannot explain the recent observations
of atmospheric neutrino mixing. However the data still allow a wide range of
energy dependences for the vacuum mixing scale, and also allow large
electron-neutrino mixing of atmospheric neutrinos. Next generation long
baseline experiments will constrain these possibilities.Comment: 27 pages, 4 figure
Hierarchical Four-Neutrino Oscillations With a Decay Option
We present a new and novel synthesis of all existing neutrino data regarding
the disappearance and appearance of and . We assume four
neutrinos: , as well as a heavier singlet neutrino
of a few eV. The latter may decay into a massless Goldstone boson (the
singlet Majoron) and a linear combination of the doublet antineutrinos. We
comment on how this scenario may be verified or falsified in future
experiments.Comment: 13 pages, no figur
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