The determination of the neutrino mass in neutrino astronomy

Details The determination of the neutrino mass in neutrino astronomy The determination of the neutrino mass in neutrino astronomy

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...218..334r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 218, no. 1-2, July 1989, p. 334-336.

Statistics

Computation

Neutrinos, Nuclear Astrophysics, Particle Mass, Supernova 1987A, Computational Astrophysics, Luminosity, Maximum Likelihood Estimates, Particle Energy

Scientific paper

The frequency distribution of emission time intervals between consecutive neutrinos from a supernova constitutes information which is complementary to that used in standard maximum likelihood analyzes. Given a realistic luminosity function, it is shown how the Gini test can be used to determine the neutrino mass from this frequency distribution. The number of SN 1987 A neutrino events seen in the Kamiokande detector are, however, too few to determine simultaneously luminosity parameters and the neutrino mass.

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