G. Gelmini et A. Kusenko, Highest-energy cosmic rays from fermi-degenerate relic neutrinos consistent with Super-Kamiokande results, PHYS REV L, 82(26), 1999, pp. 5202-5204
Relic neutrinos with mass 0.07(-0.04)(+0.02) eV, in the range consitent wit
h Super-Kamiokande data, can explain the cosmic rays with energies in exces
s of the Greisen-Zatsepin-Kuzmin cutoff. The spectrum of ultrahigh energy c
osmic rays produced in this fashion has some distinctive features that may
help identify their origin. Our mechanism does not require but is consisten
t with a neutrino density high enough to be a new kind of hot dark matter.