Cosmic-ray neutrino annihilation on relic neutrinos revisited: a mechanismfor generating air showers above the Greisen-Zatsepin-Kuzmin cutoff

If neutrinos are a significant contributor to the matter density of the uni verse, then they should have similar to eV mass and cluster in galactic (su per) cluster halos, and possibly in galactic halos as well. It was noted in the early 1980's that cosmic ray neutrinos with energy within delta E/E-R = Gamma(z)/M-z similar to 3% of the peak energy E-R = 4 (eV/m(nu)) x 10(21) eV will annihilate on the nonrelativistic relic antineutrinos (and vice ve rsa) to produce the Z-boson with an enhanced, resonant cross section of O(G (F)) similar to 10(-32) cm(2). The result of the resonant neutrino annihila tion is a hadronic Z-burst 70% of the time, which contains, on average, thi rty photons and 2.7 nucleons with energies near or above the GZK cutoff ene rgy of 5 x 10(19) eV. These photons and nucleons produced within our Superg alactic halo may easily propagate to earth and initiate super-GZK air showe rs. Here we show that the probability for each neutrino flavor at its reson ant energy to annihilate within the halo of our Supergalactic cluster is li kely within an order of magnitude of 1%, with the exact value depending on unknown aspects of neutrino mixing and relic neutrino clustering. The absol ute lower bound in a hot Big Bang universe for the probability to annihilat e within a 50 Mpc radius (roughly a nucleon propagation distance) of earth is 0.036%. From fragmentation data for Z-decay, we estimate that the nucleo ns are more energetic than the photons by a factor similar to 10. Several t ests of the hypothesis are indicated. (C) 1999 Elsevier Science B.V. All ri ghts reserved.