A semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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Revtex, 30 pages (including 13 figures); paper expanded and title slightly changed, to appear in Astroparticle Physics

Scientific paper

10.1016/j.astropartphys.2005.11.

We present a semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range. The atmospheric $\nu_{\tau}$ flux is calculated for the entire zenith angle range. This flux is contributed by the oscillations of muon neutrinos coming from the two-body $\pi, K$ decays and the three-body $\mu^{\pm}$ decays, and the intrinsic tau neutrino flux surviving the oscillations. The uncertainties in our calculations are discussed in detail. The implications of our result are also discussed.

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