The photino, the sun, and high-energy neutrinos

Details The photino, the sun, and high-energy neutrinos The photino, the sun, and high-energy neutrinos

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55..257s&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, July 8, 1985, p. 257-259.

Statistics

Computation

210

Annihilation Reactions, Milky Way Galaxy, Missing Mass (Astrophysics), Solar Neutrinos, Universe, Computational Astrophysics, Elastic Scattering, Stellar Cores

Scientific paper

If the Universe contains a nearly critical density of photinos which are also assumed to constitute the dark matter in our galactic halo, then gravitational trapping by the Sun and ensuing annihilation in the solar core yields a significant flux of ≡250-MeV neutrinos. This results in about two neutrino-induced events per kiloton-year in an underground proton-decay detector.

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