The high-energy galactic tau neutrino flux and its atmospheric background

Details The high-energy galactic tau neutrino flux and its atmospheric background The high-energy galactic tau neutrino flux and its atmospheric background

2003-11-26

arxiv.org/abs/astro-ph/0311586v1

Eur.Phys.J.C33:s959,2004

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figures, talk presented in EPS03, Aachen, Germany

Scientific paper

10.1140/epjcd/s2004-03-1844-9

We compare the tau neutrino flux arising from the galaxy and the earth atmosphere for $10^{3} \leq E/{GeV} \leq 10^{11}$. The intrinsic and oscillated tau neutrino fluxes from both sources are considered. We find that, for $E\geq 10^3$ GeV, the oscillated $\nu_{\tau}$ flux along the galactic plane dominates over the maximal intrinsic atmospheric $\nu_{\tau}$ flux, i.e., the flux along the horizontal direction. We also briefly comment on the prospects for observing these high-energy tau neutrinos.

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