Physical implications of the KAMIOKA observation of neutrinos from Supernova 1987A

Details Physical implications of the KAMIOKA observation of neutrinos from Supernova 1987A Physical implications of the KAMIOKA observation of neutrinos from Supernova 1987A

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvl..59..367a&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 59, July 20, 1987, p. 367-369.

Statistics

Computation

58

Electron Scattering, Magellanic Clouds, Neutrino Beams, Supernova 1987A, Computational Astrophysics, Cross Sections, Electron Energy, Trapped Particles

Scientific paper

It is shown that the neutrino events associated with SN 1987A are characterized by the first energetic (Eν ≡ 25 MeV) electron-capture νe pulse with quite a high source neutrino flux [Lν,e ≅ (1 - 2)×1053erg], and by the subsequent thermal pair neutrinos with a modest average energy >Eν< ≅ 7 MeV and also with a reasonable source neutrino flux Lν ≅ 3×1053erg. Some significant constraints on particle physics are also derived.

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