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arXiv · hep-ph/9403287

Neutrino Fluxes and Resonance Physics with Neutrino Telescopes

Myron Bander·H. R. Rubinstein
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Abstract

Expected atmospheric ${\bar ν_e}$ 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 $D_s^*$ 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.

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Myron Bander, H. R. Rubinstein. 1994-03-15. Neutrino Fluxes and Resonance Physics with Neutrino Telescopes. https://doi.org/10.1103/physrevd.51.1410

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