Theoretical Predictions of Ultra-High Energy Neutrino Fluxes

Details Theoretical Predictions of Ultra-High Energy Neutrino Fluxes Theoretical Predictions of Ultra-High Energy Neutrino Fluxes

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1439s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Applying our recently developed propagation code we review extragalactic neutrino fluxes above 1014 eV in various scenarios. We specifically identify scenarios in which the cosmogenic neutrino flux, produced by pion production of ultra high energy cosmic rays outside their sources, is considerably higher than the "Waxman-Bahcall bound". We also compare this flux with neutrino fluxes in top-down models, the Z -burst model and a model of new hadrons. All these fluxes allow to detect ultra-high energy neutrinos with experiments currently under construction or in the proposal stage. We also discuss the possibility to detect point-like neutrino sources.

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