2 research outputs found
Atmospheric neutrino oscillations in three-flavor neutrinos
We analyzed the atmospheric neutrino experiments of SuperKamiokande including
zenith angle dependence's using the three-flavor neutrino framework with the
hierarchy m^2_1 \approx m^2_2<<m^2_3. Taking into account the terrestrial,
solar neutrino experimental data and the atmospheric neutrino experiments
including the sub-GeV and multi-GeV data in SuperKamiokande, large angle
solution in the solar neutrino experiments is favored and the range of the mass
parameter Deltam^2_{23} is restricted between 0.08eV^2 - 2eV^2. Allowed regions
of mixing parameters are (theta_{13}<4degree, 27degree<theta_{23}< 32degree)
for Delta m_{23}^2=1eV^2 and (theta_{13}<3degree, 28degree<theta_{23}
<33degree) for Deltam_{23}^2=0.1 eV^2.Comment: 21 pages, LaTe
Future Oscillation Experiments and Present Data
Our goal in this paper is to examine the discovery potential of laboratory
experiments searching for the oscillation , in the light of recent data on solar and atmospheric neutrino
experiments, which we analyse together with the most restrictive results from
laboratory experiments on neutrino oscillations. In order to explain
simultaneously present results we use a four-neutrino framework, with an
additional sterile neutrino. Our predictions are rather pessimistic for the
upcoming experiments NOMAD and CHORUS, which, we find, are able to explore only
a small area of the oscillation parameter space. On the other hand, the
discovery potential of future experiments is much larger. We consider three
examples. E803, which is approved to operate in the future Fermilab main
injector beam line, MINOS, a proposed long-baseline experiment also using the
Fermilab beam, and NAUSICAA, an improved detector which improves by an order of
magnitude the performance of CHORUS/NOMAD and can be operated either at CERN or
at Fermilab beams. We find that those experiments can cover a very substantial
fraction of the oscillation parameter space, having thus a very good chance of
discovering and oscillation modes.Comment: Latex file using ReVTeX and epsifig.sty. 40 Pages. Revised version
includes new references and changed Fig.