Neutrino Fluxes and Resonance Physics with Neutrino Telescopes

Abstract

Expected atmospheric ${\bar{\nu }}_e$ fluxes will result in a significant number of resonantly produced low mass hadronic vector states, as the $\rho$, in large volume neutrino telescopes. The existence of sources of higher energy neutrinos will result in the production of higher mass states, as the $D_s^{\ast }$ and the $(\bar{t}b{)}_{J=1}$. 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.

Comments: pages, UCI-TR 94-10