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.
|出版狀態||Published - 16 7月 2009|
|事件||European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009 - Krakow, Poland|
持續時間: 16 7月 2009 → 22 7月 2009
|Conference||European Physical Society Europhysics Conference on High Energy Physics, EPS-HEP 2009|
|期間||16/07/09 → 22/07/09|