Characteristics of neutrino emission from the SN1987A supernova

Details Characteristics of neutrino emission from the SN1987A supernova Characteristics of neutrino emission from the SN1987A supernova

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pzetf..46..297c&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 46, Oct. 25, 1987, p. 297-300. In Russian.

Statistics

Computation

5

Gravitational Collapse, Neutrino Beams, Supernova 1987A, Antineutrinos, Computational Astrophysics

Scientific paper

Estimates of total energy input into electron antineutrinos and of the temperature and radius of the neutrinosphere of the SN1987A supernova are presented which are based on the data of four experimental facilities that have recorded neutrino emission during the star collapse. It is demonstrated that only the data provided by the Kamiokande facility are consistent with current theoretical concepts.

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