Neutrino fluxes and resonance physics with neutrino telescopes

Expected atmospheric bar νe fluxes will result in a significant number of resonantly produced low mass hadronic vector states, as the ρ, in large volume neutrino telescopes. The existence of sources of higher energy neutrinos will result in the production of higher mass states, as the Ds* and the (bar tb)J=1. We calculate the rates of production of these states and discuss their signals. Independent of theoretical flux determinations, the detection of these states will be a tool for experimentally determining these fluxes