Neutrino Fluxes and Resonance Physics with Neutrino Telescopes

Details Neutrino Fluxes and Resonance Physics with Neutrino Telescopes Neutrino Fluxes and Resonance Physics with Neutrino Telescopes

1994-03-15

arxiv.org/abs/hep-ph/9403287v1

Phys.Rev. D51 (1995) 1410-1411

Physics

High Energy Physics

High Energy Physics - Phenomenology

pages, UCI-TR 94-10

Scientific paper

10.1103/PhysRevD.51.1410

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 $D_s^*$ 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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