Atmospheric Neutrino Experiments

(2 March 2006)

First Observations of Separated Atmospheric $\nu_\mu$ and $\bar\nu_\mu$ Events in the MINOS Detector

(15 December 2005)

Evidence for an oscillatory signature in atmospheric neutrino oscillation

Super-Kamiokande Collaboration

(28 April 2004)

T. Kajita, WIN2003

(October 2003)

$ 1.3 \times 10^{-3} < \Delta{m}^2 < 3 \times 10^{-3} \, \mathrm{eV}^2 \qquad \sin^2 2\vartheta > 0.90 \qquad (90\% \mathrm{C.L.}) $

Best fit value of mixing parameters: $ \Delta{m}^2 \simeq 2.0 \times 10^{-3} \, \mathrm{eV}^2 $, $ \tan^2\vartheta \simeq 1.0 $ [Y. Hayato, EPS2003].
(July 2003)

The combined analysis of Super-Kamiokande atmospheric neutrino data in terms of two-neutrino mixing indicate that the $\nu_\mu \to \nu_\tau$ oscillation channel is favored [M. Shiozawa, Neutrino 2002].
(June 2002)

Experiments

Baksan (Home, Spires) References
Frejus (Spires) References
IMB (Home, Spires) References
Kamiokande (Home, Spires) References
MACRO (Home, Spires) References
MINOS (Home, Spires) References
NUSEX (Spires) References
Soudan 2 (Home, Spires) References
Super-Kamiokande (Home, Spires) References

Future Experiments

INO (Home

Future Projects

LAGUNA (Home, Spires) References

Neutrino Unbound

We Can Put an End to Word Attachments

Authors:
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it

Last Update: Wed 11 Apr 2012, day 102 of the year 2012, 14:48:37 UTC