| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1771606 | Astroparticle Physics | 2006 | 10 Pages |
Abstract
We present a semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range. The atmospheric ντ flux is calculated for the entire zenith angle range. This flux is contributed by the oscillations of muon neutrinos coming from the two-body π and K decays and the three-body μ± 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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Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Fei-Fan Lee, Guey-Lin Lin,