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Evidence for oscillation of atmospheric neutrinos
We present an analysis of atmospheric neutrino data from a 33.0thinspthinspktonthinspthinspyr (535-day) exposure of the Super-Kamiokande detector. The data exhibit a zenith angle dependent deficit of… Expand
Detection of the Free Neutrino: a Confirmation.
The Super-Kamiokande detector
Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons. During the period April, 1996 to July, 2001, Super-Kamiokande I collected 1678 live-days of data,… Expand
Observation of a neutrino burst from supernova SN 1987A.
DETECTION OF THE FREE ANTINEUTRINO
The antineutrino absorption reaction p( nu -bar, beta /sup +/)n was observed in two 200-liter water targets each placed between large liquid scintillation detectors and located near a powerful… Expand
On the Detection of the Free Neutrino
The experiment previously proposed [to Detect the Free Neutrino] has been initiated, with a Hanford pile as a neutrino source. It appears probable that neutrino detection has been accomplished, and… Expand
Nobel Prize for Physics
THE formulation of de Broglie's wave-particle theory in 1924 and its experimental verification in 1927 by Dr. C. J. Davisson at New York and Prof. G. P. Thomson at Aberdeen mark an outstanding epoch… Expand
Measurements of the solar neutrino flux from Super-Kamiokande's first 300 days
The first results of the solar neutrino flux measurement from Super-Kamiokande are presented. The results shown here are obtained from data taken between 31 May 1996, and 23 June 1997. Using our… Expand