We discuss the reconstruction of neutrino flavor ratios at astrophysical sources through the future neutrino-telescope measurements. We demonstrate that the accuracies in the measurements of R = φ ( nμ)/ (φ(ve) + f(Vτ)) and S = f(ve)/f(v τ) should both be better than 10% in order to distinguish between the pion source and the muon-damped source at the 3 σ level.
|Number of pages||3|
|State||Published - 1 Dec 2009|
|Event||European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009 - Krakow, Poland|
Duration: 16 Jul 2009 → 22 Jul 2009
|Conference||European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009|
|Period||16/07/09 → 22/07/09|