Implications of the supernova SN 1987A neutrino signals

Details Implications of the supernova SN 1987A neutrino signals Implications of the supernova SN 1987A neutrino signals

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..60.1789g&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 60, May 2, 1988, p. 1789-1792.

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71

Energy Spectra, Magnetic Moments, Neutrinos, Supernova 1987A, Bohr Magneton, Energetic Particles, Solar Neutrinos

Scientific paper

Neutrino events of SN 1987A observed by the Kamiokande II and Irvine-Michigan-Brookhaven (IMB) detectors have been used to constrain various neutrino parameters. It is noted that the fit of a thermal spectrum to the IMB data, which correspond to the high-energy wing of the spectrum, overestimates the effective temperature and underestimates the total energy. Bounds on the neutrino magnetic moment of between 10 to the -12th and 10 to the -13th muB are proposed. Other factors considered include the neutrino burst duration, precession in the galactic magnetic field, and the black hole possibility.

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