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Super-Kamiokande 0.07 eV Neutrinos in Cosmology: Hot Dark Matter and the Highest Energy Cosmic Rays

Graciela B. Gelmini

hep-pharXiv:hep-ph/0005263

Abstract

Relic neutrinos with mass in the range indicated by Super-Kamiokande results if neutrino masses are hierarchial (about 0.07 eV) are many times deemed too light to be cosmologically relevant. Here we remark that these neutrinos may significantly contribute to the dark matter of the Universe (with a large lepton asymmetry L) and that their existence might be revealed by the spectrum of ultra high energy cosmic rays (maybe even in the absence of a large L).

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