Neutrinos from hell

Details Neutrinos from hell Neutrinos from hell

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987s%26t....73..477s&link_type=abstract

Sky and Telescope (ISSN 0037-6604), vol. 73, May 1987, p. 477-479.

Physics

Neutrinos, Solar Neutrinos, Stellar Evolution, Antineutrinos, Cylindrical Tanks, Elementary Particles, Energetic Particles, Magellanic Clouds, Shock Waves, Supernova 1987A

Scientific paper

The detection of neutrinos is studied. The use of the Kamiokande II detector, which is a cylindrical tank holding about 3000 tons of highly purified water, for neutrino detection is examined. The operation and capabilities of the Kamiokande II detector are described. The Kamiokande II and Irvine-Michigan-Brookhaven detector observed the neutrinos from SN 1987A. The relation between the supernova and the neutrinos is analyzed. Particular consideration is given to the shock wave and the energies of the neutrinos. Additional data provided by the neutrino observations are discussed.

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